Remeis-Wiki - User contributions [en]

PhD Hat Caro

2025-08-28T08:40:02Z

Zainab: /* Ideas for Caro's PhD hat go here! */

[[Category:internal]]
=Ideas for Caro's PhD hat go here! =

- obviously something with steam locomotives, maybe get a small paper version for the hat?

- Slurm queue printout?

- something about tea, teapots (e.g. a metric of a teapot?)
(can be merged with her pottery hobby, maybe a coffee mug?)

- a open fire with a turnable Nico figure above the flame

- rotating fish and brainrot memes

- DPREAO president including laws, Kim Jung Un meme, battle and war with anti-dpreao coalition

- a hammock maybe as a tassel?

- a little banana pizza?

- wanted signs for slurm offenders with a nerf stuck on it

- french press / fancy coffee

PhD Hat Caro

2025-08-28T07:53:00Z

Zainab: /* Ideas for Caro's PhD hat go here! */

Litclub

2024-12-17T13:00:25Z

Zainab: /* Frequently Asked Questions */

== What is LitClub? ==

LitClub is a weekly meeting held at the Dr. Karl Remeis Observatory for all observatory members. The meeting consists of a presentation of a scientific, astrophysics-related paper chosen by a speaker, who was selected to give a talk for the current week and is followed by a general discussion. The goals of the meeting are the following:

* to improve communication and presentation skills for bachelor, master, and PhD students
* to provide a platform for free and casual discussion of scientific topics
* to learn more ;-)
* to bring all our groups together

LitClub takes place on Tuesdays at 11:30, in the conference room in the main observatory building, or (if there are too many attendees) in the library in the meridian building.

LitClub is a mandatory activity for all observatory members. All students are on the list of presenters. All postdocs are expected to contribute to the discussion and to take over the presentation in case the speaker has to cancel last minute.

Please find below the general rules and commonly asked questions.

== Organization ==

Every week a person is chosen to present a paper.

'''How's the presenter chosen?'''

The selection of a presenter is done semi-randomly by Ingo, taking information about people's availability into account. At the beginning of the semester, a table is sent around where you can enter your availability during certain weeks (yes, all students are expected to be available a respectable amount of weeks per semester to make a presentation). If an observatory member provided no information in the table, the LitClub organizers assume that this person is available on any given day. The presenter is informed about the presentation a few days in advance.

'''How's the paper to be presented chosen?'''

A presenter chooses a paper from recently published papers or a list of somewhat interesting papers below, which contain the classical ("must-read") astrophysics-related papers, as well as some new advances in the field. A different paper can be chosen, either from a peer-reviewed journal or arxiv. It is expected that it is related to space science (including, e.g., planetary science, instruments, methods, ...). In case you want to present something different, for example, to talk about your past or present research, please inform the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].

'''The best way''' to select a paper is to check [https://arxiv.org arxiv] 2 weeks before the day of your presentation. '''Only''' if you do not find anything suitable there check the list given below for a paper. If you do select a paper from the list '''make sure to inform the litclub organizers''' well in advance so it can be checked that the paper was not already presented.

'''How's the presentation done?'''

Presentation at the LitClub requires a few prepared slides with the most essential information, which helps to guide you (and your audience) through your talk. Any time-consuming design features are strongly discouraged: you are expected to quickly prepare simple slides with valuable content. See below the section on "Guidelines" for more details on how long the talk should be etc.

== Guidelines and Information ==

'''Basic guidelines and information on the purpose of the litclub, the roles of the audience and the speaker, and how to prepare and present the talk were presented in a short talk (by Thomas Dauser), which you can find here: [[File:litclub_guidelines.pdf]]'''

If you are new to the litclub, it is very helpful to have a look there, as it is currently the most detailed resource of information on how the litclub works.

== Frequently Asked Questions ==

'''Is it really mandatory for all students?'''

Yes.

'''What if I cannot present when I am asked?'''

In this case, you have to find a person who could present instead of you on the date. At the same time, you are expected to give a presentation within the following weeks.

'''What are acceptable reasons to not present, when asked?'''

Lectures and examinations (confirmed by schedule) or vacation and sickness (confirmed with your supervisor). In the case of one of these reasons, please see the previous question. If you got sick on the day of the presentation and there was no time to find a different speaker, you will be shifted to one of the following weeks and LitClub will be conducted by one (or a few) of the observatory postdocs.

'''I have an upcoming conference talk, is it a good reason to not present at LitClub a week before?'''

No. It is expected that the LitClub will not take too much of your preparation time. If it does - you need (want) to learn how to make it quicker, which is possible only by practice.

'''I am working on my master (bachelor/PhD) thesis, is it an acceptable reason to not present at LitClub?'''

No. Only if you have your defence within a few days of the LitClub in question. Otherwise: it is the time for you to work with a lot of literature. Just pick one of the papers you recently read for your thesis and present it.

'''Do I need slides for the presentation'''

Yes. The current request by our professors is that you would prepare simple slides with the main information. (5 slides is plenty).

'''How much time am I expected to spend to prepare for the LitClub presentation?'''

It depends on the paper you choose, but in general, you should be able to prepare your talk within half a working day.

== Contact ==

For questions and comments, please contact the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].
Any major modifications to the structure of LitClub will be discussed with the professors.

== Litclub Paper List (WILL BE UPDATED!!!)==

We collect potentially interesting papers in an [https://ui.adsabs.harvard.edu/user/libraries/8mOwkXjvQl206110FBulVw ADS library] to give some inspiration. But be reminded that you should check new publications first before consulting this list. Also, if you select a paper from this list '''inform the organizers as soon as possible''' so it can be checked for duplicates. It is also particularly encouraged to present any interesting scientific work, not restricted to astronomy! Also, in case you found interesting papers feel free to add them to the list below (create sections as required, beware that this page is not updated as often as it should be so the chance that they have been presented already is rather high).

''On a best effort basis we maintain an second [https://ui.adsabs.harvard.edu/user/libraries/9B-WkBVbTAmnzI7rmQ7dtA ADS (presented) library] where already presented papers are listed.''

=== X-ray astronomy ===

- Electromagnetic extraction of energy from Kerr black holes (Blandford-Znajek mechanism): Blandford, Znajek, MNRAS 179, 433, 1977 <ref>[https://ui.adsabs.harvard.edu/abs/1977MNRAS.179..433B/abstract]Blandford, Znajek, MNRAS 179, 433, 1977</ref> (although, astrophysically, the Blandford-Payne mechanism likely contributes more to jet launching, e.g., Livio, Ogilvie, Pringle, ApJ 512, 100, 1999)

- "The corona contracts in a black-hole transient": Kara et al., Nature 565 198, 2019 <ref>[https://ui.adsabs.harvard.edu/abs/2019Natur.565..198K/abstract]Kara et al., Nature 565 198, 2019</ref>, although this result is disputed (e.g., arxiv/2112.08116)

- Connection of FRBs and magnetars: "INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154" (Mereghetti, 2020ApJ...898L..29M)

- "Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT" (Ma et al., 2021NatAs...5...94M)

- "Cygnus X-1 contains a 21-solar mass black hole—Implications for massive star winds" (Miller-Jones 2021Sci...371.1046M)

- EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade (Batista et al., arxiv.org/abs/2110.10074) - perhaps too long but really interesting summary

- Dark Energy Survey 3 Year Results (e.g., http://adsabs.harvard.edu/abs/2021arXiv210513549D)

=== Aliens? :0 ===

- Estimating the prevalence of malicious extraterrestrial civilizations (Caballero 2022arXiv220511618C) [https://arxiv.org/pdf/2205.11618.pdf]

=== Cosmology ===

- Is the Expansion of the Universe Accelerating? All Signs Still Point to Yes: A Local Dipole Anisotropy Cannot Explain Dark Energy [https://iopscience.iop.org/article/10.3847/1538-4357/ab7a16/pdf]

=== Statistics ===

- "STATISTICS, HANDLE WITH CARE: DETECTING MULTIPLE MODEL COMPONENTS WITH THE LIKELIHOOD RATIO TEST" (Protassov, 2002ApJ...571..545P)

=== Some more extravagant stuff ===

- The Breakthrough Listen Search For Intelligent Life Near the Galactic Center (Gajjar et al., ApJ 162, 33, 2021)

- An Objective Bayesian Analysis of Life's Early Start and Our Late Arrival (Kipping, 2020, https://arxiv.org/abs/2005.09008)

=== Non-astrophysics ===

- creating unique random numbers using the quantum noise of the vacuum: Gabriel et al., Nature Photonics 4, 711, 2010

Litclub

2024-12-17T12:52:34Z

Zainab: /* Organization */

== What is LitClub? ==

LitClub is a weekly meeting held at the Dr. Karl Remeis Observatory for all observatory members. The meeting consists of a presentation of a scientific, astrophysics-related paper chosen by a speaker, who was selected to give a talk for the current week and is followed by a general discussion. The goals of the meeting are the following:

* to improve communication and presentation skills for bachelor, master, and PhD students
* to provide a platform for free and casual discussion of scientific topics
* to learn more ;-)
* to bring all our groups together

LitClub takes place on Tuesdays at 11:30, in the conference room in the main observatory building, or (if there are too many attendees) in the library in the meridian building.

LitClub is a mandatory activity for all observatory members. All students are on the list of presenters. All postdocs are expected to contribute to the discussion and to take over the presentation in case the speaker has to cancel last minute.

Please find below the general rules and commonly asked questions.

== Organization ==

Every week a person is chosen to present a paper.

'''How's the presenter chosen?'''

The selection of a presenter is done semi-randomly by Ingo, taking information about people's availability into account. At the beginning of the semester, a table is sent around where you can enter your availability during certain weeks (yes, all students are expected to be available a respectable amount of weeks per semester to make a presentation). If an observatory member provided no information in the table, the LitClub organizers assume that this person is available on any given day. The presenter is informed about the presentation a few days in advance.

'''How's the paper to be presented chosen?'''

A presenter chooses a paper from recently published papers or a list of somewhat interesting papers below, which contain the classical ("must-read") astrophysics-related papers, as well as some new advances in the field. A different paper can be chosen, either from a peer-reviewed journal or arxiv. It is expected that it is related to space science (including, e.g., planetary science, instruments, methods, ...). In case you want to present something different, for example, to talk about your past or present research, please inform the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].

'''The best way''' to select a paper is to check [https://arxiv.org arxiv] 2 weeks before the day of your presentation. '''Only''' if you do not find anything suitable there check the list given below for a paper. If you do select a paper from the list '''make sure to inform the litclub organizers''' well in advance so it can be checked that the paper was not already presented.

'''How's the presentation done?'''

Presentation at the LitClub requires a few prepared slides with the most essential information, which helps to guide you (and your audience) through your talk. Any time-consuming design features are strongly discouraged: you are expected to quickly prepare simple slides with valuable content. See below the section on "Guidelines" for more details on how long the talk should be etc.

== Guidelines and Information ==

'''Basic guidelines and information on the purpose of the litclub, the roles of the audience and the speaker, and how to prepare and present the talk were presented in a short talk (by Thomas Dauser), which you can find here: [[File:litclub_guidelines.pdf]]'''

If you are new to the litclub, it is very helpful to have a look there, as it is currently the most detailed resource of information on how the litclub works.

== Frequently Asked Questions ==

'''Is it really mandatory for all students?'''

Yes.

'''What if I cannot present when I am asked?'''

In this case, you have to find a person who could present instead of you on the date. At the same time, you are expected to give a presentation within the following weeks.

'''What are acceptable reasons to not present, when I was asked?'''

Lectures and examinations - confirmed by schedule or vacation and sickness - confirmed with your supervisor. In the case of one of these reasons, please see the previous question. If you got sick on the day of the presentation and there was no time to find a different speaker, you will be shifted to one of the following weeks and LitClub will be conducted by one (or a few) of the observatory postdocs.

'''I have an upcoming conference talk, is it a good reason to not present at LitClub a week before?'''

No. It is expected that the LitClub will not take too much of your preparation time. If it does - you need (want) to learn how to make it quicker, which is possible only by practice.

'''I am working on my master (bachelor/PhD) thesis, is it an acceptable reason to not present at LitClub?'''

No. Only if you have your defence within a few days of the LitClub in question. Otherwise: it is the time for you to work with a lot of literature. Just pick one of the papers you recently read for your thesis and present it.

'''Do I have to have slides for the presentation'''

Yes. The current request by our professors is that you would prepare simple slides with the main information. (5 slides is plenty)

'''How much time I am expected to spend to prepare for the LitClub presentation?'''

It depends on the paper you choose, but in general, you should be able to prepare your talk within half of a working day.

== Contact ==

For questions and comments, please contact the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].
Any major modifications to the structure of LitClub will be discussed with the professors.

== Litclub Paper List (WILL BE UPDATED!!!)==

We collect potentially interesting papers in an [https://ui.adsabs.harvard.edu/user/libraries/8mOwkXjvQl206110FBulVw ADS library] to give some inspiration. But be reminded that you should check new publications first before consulting this list. Also, if you select a paper from this list '''inform the organizers as soon as possible''' so it can be checked for duplicates. It is also particularly encouraged to present any interesting scientific work, not restricted to astronomy! Also, in case you found interesting papers feel free to add them to the list below (create sections as required, beware that this page is not updated as often as it should be so the chance that they have been presented already is rather high).

''On a best effort basis we maintain an second [https://ui.adsabs.harvard.edu/user/libraries/9B-WkBVbTAmnzI7rmQ7dtA ADS (presented) library] where already presented papers are listed.''

=== X-ray astronomy ===

- Electromagnetic extraction of energy from Kerr black holes (Blandford-Znajek mechanism): Blandford, Znajek, MNRAS 179, 433, 1977 <ref>[https://ui.adsabs.harvard.edu/abs/1977MNRAS.179..433B/abstract]Blandford, Znajek, MNRAS 179, 433, 1977</ref> (although, astrophysically, the Blandford-Payne mechanism likely contributes more to jet launching, e.g., Livio, Ogilvie, Pringle, ApJ 512, 100, 1999)

- "The corona contracts in a black-hole transient": Kara et al., Nature 565 198, 2019 <ref>[https://ui.adsabs.harvard.edu/abs/2019Natur.565..198K/abstract]Kara et al., Nature 565 198, 2019</ref>, although this result is disputed (e.g., arxiv/2112.08116)

- Connection of FRBs and magnetars: "INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154" (Mereghetti, 2020ApJ...898L..29M)

- "Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT" (Ma et al., 2021NatAs...5...94M)

- "Cygnus X-1 contains a 21-solar mass black hole—Implications for massive star winds" (Miller-Jones 2021Sci...371.1046M)

- EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade (Batista et al., arxiv.org/abs/2110.10074) - perhaps too long but really interesting summary

- Dark Energy Survey 3 Year Results (e.g., http://adsabs.harvard.edu/abs/2021arXiv210513549D)

=== Aliens? :0 ===

- Estimating the prevalence of malicious extraterrestrial civilizations (Caballero 2022arXiv220511618C) [https://arxiv.org/pdf/2205.11618.pdf]

=== Cosmology ===

- Is the Expansion of the Universe Accelerating? All Signs Still Point to Yes: A Local Dipole Anisotropy Cannot Explain Dark Energy [https://iopscience.iop.org/article/10.3847/1538-4357/ab7a16/pdf]

=== Statistics ===

- "STATISTICS, HANDLE WITH CARE: DETECTING MULTIPLE MODEL COMPONENTS WITH THE LIKELIHOOD RATIO TEST" (Protassov, 2002ApJ...571..545P)

=== Some more extravagant stuff ===

- The Breakthrough Listen Search For Intelligent Life Near the Galactic Center (Gajjar et al., ApJ 162, 33, 2021)

- An Objective Bayesian Analysis of Life's Early Start and Our Late Arrival (Kipping, 2020, https://arxiv.org/abs/2005.09008)

=== Non-astrophysics ===

- creating unique random numbers using the quantum noise of the vacuum: Gabriel et al., Nature Photonics 4, 711, 2010

Litclub

2024-12-17T12:52:21Z

Zainab: /* Organization */

== What is LitClub? ==

LitClub is a weekly meeting held at the Dr. Karl Remeis Observatory for all observatory members. The meeting consists of a presentation of a scientific, astrophysics-related paper chosen by a speaker, who was selected to give a talk for the current week and is followed by a general discussion. The goals of the meeting are the following:

* to improve communication and presentation skills for bachelor, master, and PhD students
* to provide a platform for free and casual discussion of scientific topics
* to learn more ;-)
* to bring all our groups together

LitClub takes place on Tuesdays at 11:30, in the conference room in the main observatory building, or (if there are too many attendees) in the library in the meridian building.

LitClub is a mandatory activity for all observatory members. All students are on the list of presenters. All postdocs are expected to contribute to the discussion and to take over the presentation in case the speaker has to cancel last minute.

Please find below the general rules and commonly asked questions.

== Organization ==

Every week a person is chosen to present a paper.

'''How's the presenter chosen?'''

The selection of a presenter is done semi-randomly by Ingo, taking information about people's availability into account. At the beginning of the semester, a table is sent around where you can enter your availability during certain weeks (yes, all students are expected to be available a respectable amount of weeks per semester to make a presentation). If an observatory member provided no information in the table, the LitClub organizers assume that this person is available on any given day. The presenter is informed about the presentation a few days in advance.

'''How's the paper to be presented chosen?'''

A presenter chooses a paper from recently published papers or a list of somewhat interesting papers below, which contain the classical ("must-read") astrophysics-related papers, as well as some new advances in the field. A different paper can be chosen, either from a peer-reviewed journal or arxiv. It is expected that it is related to space science (including, e.g., planetary science, instruments, methods, ...). In case you want to present something different, for example, to talk about your past or present research, please inform the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].

'''The best way''' to select a paper is to check [https://arxiv.org arxiv] 2 weeks before the day of your presentation. '''Only''' if you do not find anything suitable there check the list given below for a paper. If you do select a paper from the list '''make sure to inform the litclub organizers''' well in advance so it can be checked that the paper was not already presented.

'''How's the presentation done?'''
Presentation at the LitClub requires a few prepared slides with the most essential information, which helps to guide you (and your audience) through your talk. Any time-consuming design features are strongly discouraged: you are expected to quickly prepare simple slides with valuable content. See below the section on "Guidelines" for more details on how long the talk should be etc.

== Guidelines and Information ==

'''Basic guidelines and information on the purpose of the litclub, the roles of the audience and the speaker, and how to prepare and present the talk were presented in a short talk (by Thomas Dauser), which you can find here: [[File:litclub_guidelines.pdf]]'''

If you are new to the litclub, it is very helpful to have a look there, as it is currently the most detailed resource of information on how the litclub works.

== Frequently Asked Questions ==

'''Is it really mandatory for all students?'''

Yes.

'''What if I cannot present when I am asked?'''

In this case, you have to find a person who could present instead of you on the date. At the same time, you are expected to give a presentation within the following weeks.

'''What are acceptable reasons to not present, when I was asked?'''

Lectures and examinations - confirmed by schedule or vacation and sickness - confirmed with your supervisor. In the case of one of these reasons, please see the previous question. If you got sick on the day of the presentation and there was no time to find a different speaker, you will be shifted to one of the following weeks and LitClub will be conducted by one (or a few) of the observatory postdocs.

'''I have an upcoming conference talk, is it a good reason to not present at LitClub a week before?'''

No. It is expected that the LitClub will not take too much of your preparation time. If it does - you need (want) to learn how to make it quicker, which is possible only by practice.

'''I am working on my master (bachelor/PhD) thesis, is it an acceptable reason to not present at LitClub?'''

No. Only if you have your defence within a few days of the LitClub in question. Otherwise: it is the time for you to work with a lot of literature. Just pick one of the papers you recently read for your thesis and present it.

'''Do I have to have slides for the presentation'''

Yes. The current request by our professors is that you would prepare simple slides with the main information. (5 slides is plenty)

'''How much time I am expected to spend to prepare for the LitClub presentation?'''

It depends on the paper you choose, but in general, you should be able to prepare your talk within half of a working day.

== Contact ==

For questions and comments, please contact the organizers: [mailto:astro-literature@lists.fau.de astro-literature@lists.fau.de].
Any major modifications to the structure of LitClub will be discussed with the professors.

== Litclub Paper List (WILL BE UPDATED!!!)==

We collect potentially interesting papers in an [https://ui.adsabs.harvard.edu/user/libraries/8mOwkXjvQl206110FBulVw ADS library] to give some inspiration. But be reminded that you should check new publications first before consulting this list. Also, if you select a paper from this list '''inform the organizers as soon as possible''' so it can be checked for duplicates. It is also particularly encouraged to present any interesting scientific work, not restricted to astronomy! Also, in case you found interesting papers feel free to add them to the list below (create sections as required, beware that this page is not updated as often as it should be so the chance that they have been presented already is rather high).

''On a best effort basis we maintain an second [https://ui.adsabs.harvard.edu/user/libraries/9B-WkBVbTAmnzI7rmQ7dtA ADS (presented) library] where already presented papers are listed.''

=== X-ray astronomy ===

- Electromagnetic extraction of energy from Kerr black holes (Blandford-Znajek mechanism): Blandford, Znajek, MNRAS 179, 433, 1977 <ref>[https://ui.adsabs.harvard.edu/abs/1977MNRAS.179..433B/abstract]Blandford, Znajek, MNRAS 179, 433, 1977</ref> (although, astrophysically, the Blandford-Payne mechanism likely contributes more to jet launching, e.g., Livio, Ogilvie, Pringle, ApJ 512, 100, 1999)

- "The corona contracts in a black-hole transient": Kara et al., Nature 565 198, 2019 <ref>[https://ui.adsabs.harvard.edu/abs/2019Natur.565..198K/abstract]Kara et al., Nature 565 198, 2019</ref>, although this result is disputed (e.g., arxiv/2112.08116)

- Connection of FRBs and magnetars: "INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154" (Mereghetti, 2020ApJ...898L..29M)

- "Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT" (Ma et al., 2021NatAs...5...94M)

- "Cygnus X-1 contains a 21-solar mass black hole—Implications for massive star winds" (Miller-Jones 2021Sci...371.1046M)

- EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade (Batista et al., arxiv.org/abs/2110.10074) - perhaps too long but really interesting summary

- Dark Energy Survey 3 Year Results (e.g., http://adsabs.harvard.edu/abs/2021arXiv210513549D)

=== Aliens? :0 ===

- Estimating the prevalence of malicious extraterrestrial civilizations (Caballero 2022arXiv220511618C) [https://arxiv.org/pdf/2205.11618.pdf]

=== Cosmology ===

- Is the Expansion of the Universe Accelerating? All Signs Still Point to Yes: A Local Dipole Anisotropy Cannot Explain Dark Energy [https://iopscience.iop.org/article/10.3847/1538-4357/ab7a16/pdf]

=== Statistics ===

- "STATISTICS, HANDLE WITH CARE: DETECTING MULTIPLE MODEL COMPONENTS WITH THE LIKELIHOOD RATIO TEST" (Protassov, 2002ApJ...571..545P)

=== Some more extravagant stuff ===

- The Breakthrough Listen Search For Intelligent Life Near the Galactic Center (Gajjar et al., ApJ 162, 33, 2021)

- An Objective Bayesian Analysis of Life's Early Start and Our Late Arrival (Kipping, 2020, https://arxiv.org/abs/2005.09008)

=== Non-astrophysics ===

- creating unique random numbers using the quantum noise of the vacuum: Gabriel et al., Nature Photonics 4, 711, 2010

List of symbiotic X-ray binaries

2024-02-21T12:47:49Z

Zainab:

{| class="wikitable"
! Source Name
! Optical Sp/type
! L/HMXB Class
! Luminosity (erg/s)
! Spin Period (sec)
! Orbital Period (days)
! CRSF Energies (keV)
! Reference
|-
| [[3A 1954+319]]
| RSG
| HMXB
| 4e32 - 1e35
| 1.91e4
|
|
| <ref name="Farrell10a" />,<ref name="Masetti07a" />
|-
| [[GX 1+4]]
|
|
| 1e37
| 120
| 304
|
| <ref name="Farrell10a" />,<ref name="Masetti07a" />
|-
| [[4U 1700+24]]
|
|
| 2e32 - 1e34
| 404
|
|
| <ref name="Farrell10a" />,<ref name="Masetti07a" />
|-
| [[Sct X-1]]
| Mira variable
| LMXB
| 2e34?
| 112
|
|
| <ref name="Farrell10a" />,<ref name="Masetti07a" />
|-
| [[1RXS J180431.1-273932]]
|
|
| <6e34
| 494
|
|
| <ref name="Nucita07a" />
|-
| [[IGR J16194-2810]]
|
|
| 1.4e35
| --
| --
| --
| <ref name="Masetti07a" />
|-
| [[IGR J16358-4726]]
|
|
|
| 5880
| --
| --
| <ref name="Nespoli09a" />
|-
| [[IGR J16393-4643]]
|
|
|
| 912.0
| 3.7
|
|
|-
| [[XTE J1743-363]]
|
|
| ?
| ?
| ?
| ?
|
|-
| [[AX J1659.0−4208]]
|
|
|
|
|
|
|
|-
| [[IGR J17407−2808]]
|
|
|
|
|
|
|
|-
| [[CXO 174528.79–290942.8]]
| RSG
| HMXB
|
|
|
|
|
|}

Zainab:

[[Category:Internal]]
'''Info'''

'''Hat:'''

30x30cm platform (top), 15cm tube (base) Umfang: ??cm -> Steven

'''General:'''
*social media
*insta walk
*Bernreuther Dominic Social Media (BDSM) → Steven
*tours and desperate wish to find a new guide planetarium half globe with clay planets → Aafia
*CCD
*FRANCI (logo) → Steven
*Christmass party (wok)
*2bros and scam
*V2 rocket → Steven
*car ford ka → knunchkugle (spherical car)
* Australia, Norway, fire etc.
* meeting Manami in the bakery

'''science:'''

*training → lightbulbe
*Machine learning → pins colored representing layers of neural network connected with strings → Jonathan,Ole
*Bscan (actual Bee ) → Amy
*Bscam (Bubble Scanning Algorith [Module] Music) → Federico drive
*B - scam (scam emails) → Caro (/home/collischon/Documents/scammails.txt)
*bubble plastic with pictures of SNR → Jonathan
*soap bubbles as a tassle → Ole
*barcode scanner → Philipp
*blazar image (in the kitchen) → Steven

'''Personal:'''
*Remeis coint (crypto currency) → Philipp
*?girlfriend has mushrooms he don't?
*mushroom picture, many mushrooms find the SNR (?)
*singing metal (tiny microphone)
*or playing metal (mini instruments) →
*container houses
*tiny houses around the word
*mountain bike
*motor bike (suzuki (susi)) mini models, probably 1st gen (1999—2002) SV650
*whiskey
*limoncello → paper bottle with bright yellow
*riesen (big riesen packed in another big riesen) (bunch of riesen that are found insted of the bubble) → Martin
*(horrible)chicken at the Rewe

[[Category:Internal]]

2023-11-16T11:08:14Z

Zainab:

Be stars in Gaia

2023-11-16T11:00:23Z

Zainab: Created page with "Gaia typically lists G-band apparent magnitude, as well as BP and RP colours. Using these, one can verify the position of the Be star on the HR diagram. Typically, the liste..."

Gaia typically lists G-band apparent magnitude, as well as BP and RP colours. Using these, one can verify the position of the Be star on the HR diagram.

Typically, the listed magnitudes need to be corrected for reddening. The amount of reddening can be approximated through an absorption coefficient Av (Ag - Gaia band), that can be estimated from the fitted Nh obtained through X-ray spectral fitting (or the nh query on HEASARC). See [https://ui.adsabs.harvard.edu/abs/2009MNRAS.400.2050G/abstract here] for example.

Be X-ray Binaries

2023-11-16T10:54:28Z

Zainab:

[[Category:Accreting X-ray Pulsars]]

Be/X-ray binary systems form the majority of accreting X-ray pulsars. In these systems the optical companion is a giant star which besides a fast low-density wind also show an equatorial disk or flattened envelope in fast rotation. This disk shows up through [http://en.wikipedia.org/wiki/Balmer_lines Balmer emission lines] (see, e.g., [http://www.astrosurf.com/~buil/us/bestar.htm The spectroscopic Be stars Atlas]. The X-ray emitting object is usually a neutron star on an eccentric orbit (e=0.1-0.9). For a recent review of Be/X-ray binaries see Reig et al. (2011)<ref name = "Reig2011a" />.

Most Be/X-ray binaries show transient activity and only very weak emission outside outbursts. Stella et al. (1986)<ref name = "Stella1986a" /> have classified the different outbursts in two types: Type I are periodical outbursts linked to the periastron passage of the neutron star and relatively short; Type II are larger outbursts with no clear link to the orbital phase.

Historically, type I outbursts have been explained by a simple picture of the passage of the neutron star through the equatorial disk of the Be star every orbit. But this picture fails to explain the large variety of outbursts seen in many systems with periods of regular outbursts, occasional giant outbursts, but also extended periods of quiescence. A possible explanation was given by the [http://harmas.arc.hokkai-s-u.ac.jp/~okazaki/BeX/index.html model developed by Atsuo Okazaki] in which the disk around the Be star will often be truncated due to tidal interactions and outbursts are triggered by changes in the disk. This model has been published in Negueruela & Okazaki 2001<ref name = "Negueruela2001a" />, Negueruela et al. (2001)<ref name = "Negueruela2001b" />, and Okazaki & Negueruela (2001)<ref name = "Okazaki2001a" />.

Sometimes, optical information can prove quite useful while studying BeXRBs. Check [[Be stars in Gaia]] for a few simple checks.

[http://integral.esac.esa.int/bexrbmonitor/webpage_oneplot.php The BeXRB Monitor] page collects data from different monitoring missions and shows current activity for a variety of sources.

See [[List of Be X-ray Binaries]] for details about individual sources.

List of accreting X-ray pulsars

2023-11-14T15:00:13Z

Zainab: /* Updated list of accreting X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars (pulse profile extractions) =

This is a list to organize a library of pulse profiles for many of the known accreting X-ray pulsars. For this we scanned the NuSTAR archive at [https://heasarc.gsfc.nasa.gov/docs/archive.html Heasarc] for all objects that are listed in the two [http://astro.uni-tuebingen.de/~xrbcat/ XRB catalogues]. All public obsids are downloaded to `/userdata/data/stierhof/pp-class/<object_name>/<obsid>`. This is more than 350 observations! After reprocessing (this creates a folder `reprocessed` in each obsid folder) the region files have to be created. Right now we are not interested in detailed analysis and for bright outbursts the region choice is not that important. If you want to contribute, please create '''one''' region file for the source and '''one''' for the background. The source should be a circle centered around the brightest part of the image. The background should be an annulus with inner radius as large as the source region, and the outer as large as possible. The source and background region files should be stored in the `reprocessed` folder as `src.reg` and `bkg.reg`. '''Note:''' The regions must be valid for both detector modules!

Once the region files are created it is straight forward to automatically extract all dataset. So please don't change anything else in the folder just yet. You can check the table if the data has been prepared (that is, if the `reprocessed` folder exists) and add the region files. If you do, please indicate it in the corresponding line in the table (searching for the source name should be helpful here).

Once we have all region files collected we can extract the pulse profiles!

{| class=wikitable
! Source
! Class
! Assignee
! Pulse Period
! Has Region
! Is Prepared
! Is Processed
|-
| [[1A 0535+262]]
| HMXB
|
| 103.47
|
|
|
|-
| [[1E 1145.1-6141]]
| HMXB
| Vicente
| 298.0
|
|
|
|-
| [[2RXP J130159.6-635806]]
| HMXB
|
| 643.0
|
|
|
|-
| [[2S 0114+650]]
| HMXB
|
| 10008.0
|
|
|
|-
| [[2S 1417-624]]
| HMXB
|
| 17.6
|
|
|
|-
| [[2S 1553-542]]
| HMXB
|
| 9.28
|
|
|
|-
| [[2S 1845-024]]
| HMXB
|
| 94.72
|
|
|
|-
| [[3A 1822-371]]
| LMXB
|
| 0.59
|
|
|
|-
| [[3U 1223-62]]
| HMXB
|
| 696.0
|
|
|
|-
| [[3U 1258-61]]
| HMXB
|
| 272.0
|
|
|
|-
| [[4U 0115+63]]
| HMXB
|
| 3.61
|
|
|
|-
| [[4U 0352+309]]
| HMXB
| Aafia
| 837.67
|
|
|
|-
| [[4U 0614+09]]
| LMXB
|
| 0.0020964360587002098
|
|
|
|-
| [[4U 1538-52]]
| HMXB
| Aafia
| 526.42
|
|
|
|-
| [[4U 1608-52]]
| LMXB
|
| 0.0016
|
|
|
|-
| [[4U 1626-67]]
| LMXB
|
| 7.7
|
|
|
|-
| [[4U 1636-536]]
| LMXB
|
| 0.001721
|
|
|
|-
| [[4U 1702-429]]
| LMXB
|
| 0.00303
|
|
|
|-
| [[4U 1728-34]]
| LMXB
|
| 0.0027548209366391185
|
|
|
|-
| [[4U 1901+03]]
| HMXB
|
| 2.76
|
|
|
|-
| [[4U 1907+09]]
| HMXB
| Aafia
| 438.0
|
|
|
|-
| [[4U 1909+07]]
| HMXB
| Aafia
| 603.6
|
|
|
|-
| [[4U 1915-05]]
| LMXB
|
| 0.0037
|
|
|
|-
| [[4U 1954+31]]
| HMXB
|
| 19400.0
|
|
|
|-
| [[4U 2206+54]]
| HMXB
|
| 5555.0
|
|
|
|-
| [[Aql X-1]]
| LMXB
|
| 0.00182
|
|
|
|-
| [[BSD 24-491]]
| HMXB
|
| 202.5
|
|
|
|-
| [[CXOGlb J174852.7-202124]]
| LMXB
|
| 0.004857
|
|
|
|-
| [[Cen X-3]]
| HMXB
|
| 4.8
|
|
|
|-
| [[Cep X-4]]
| HMXB
|
| 65.35
|
|
|
|-
| [[EXO 0748-676]]
| LMXB
|
| 0.0019157088122605363
|
|
|
|-
| [[EXO 2030+375]]
| HMXB
|
| 41.31
|
|
|
|-
| [[GRO J1008-57]]
| HMXB
| Aafia
| 93.5
|
|
|
|-
| [[GRO J1744-28]]
| LMXB
|
| 0.467
|
|
|
|-
| [[GRO J1750-27]]
| HMXB
|
| 4.45
|
|
|
|-
| [[GRO J2058+42]]
| HMXB
|
| 195.25
|
|
|
|-
| [[GRS 1741.9-2853]]
| LMXB
|
| 0.001697792869269949
|
|
|
|-
| [[GX 1+4]]
| LMXB
|
| 138.17
|
|
|
|-
| [[Ginga 0834-430]]
| HMXB
|
| 12.3
|
|
|
|-
| [[HD 110432]]
| HMXB
|
| 14200.0
|
|
|
|-
| [[HD 77581]]
| HMXB
|
| 283.0
|
|
|
|-
| [[Her X-1]]
| LMXB
|
| 1.24
|
|
|
|-
| [[IGR J00291+5934]]
| LMXB
|
| 0.00167
|
|
|
|-
| [[IGR J06074+2205]]
| HMXB
|
| 373.2
|
|
|
|-
| [[IGR J11215-5952]]
| HMXB
|
| 186.8
|
|
|
|-
| [[IGR J16320-4751]]
| HMXB
|
| 1308.8
|
|
|
|-
| [[IGR J16358-4726]]
| LMXB
|
| 5880.0
|
|
|
|-
| [[IGR J16393-4643]]
| HMXB
| Aafia
| 908.79
|
|
|
|-
| [[IGR J16418-4532]]
| HMXB
| Aafia
| 1246.0
|
|
|
|-
| [[IGR J16493-4348]]
| HMXB
|
| 1093.1
|
|
|
|-
| [[IGR J16597-3704]]
| LMXB
|
| 0.00951
|
|
|
|-
| [[IGR J17062-6143]]
| LMXB
| Vicente
| 0.00611
|
|
|
|-
| [[IGR J17329-2731]]
| LMXB
|
| 6680.0
|
|
|
|-
| [[IGR J17379-3747]]
| LMXB
| Vicente
| 0.002136
|
|
|
|-
| [[IGR J17480-2446]]
| LMXB
|
| 0.09054
|
|
|
|-
| [[IGR J17494-3030]]
| LMXB
|
| 0.002659219644588837
|
|
|
|-
| [[IGR J17498-2921]]
| LMXB
|
| 0.002494
|
|
|
|-
| [[IGR J17511-3057]]
| LMXB
|
| 0.00408
|
|
|
|-
| [[IGR J17544-2619]]
| HMXB
|
| 71.49
|
|
|
|-
| [[IGR J17591-2342]]
| LMXB
|
| 0.001897
|
|
|
|-
| [[IGR J18027-2016]]
| HMXB
|
| 139.6
|
|
|
|-
| [[IGR J18219-1347]]
| HMXB
|
| 52.46
|
|
|
|-
| [[IGR J18245-2452]]
| LMXB
|
| 0.00393
|
|
|
|-
| [[IGR J19294+1816]]
| HMXB
|
| 12.44
|
|
|
|-
| [[IGR J21343+4738]]
| HMXB
|
| 322.7
|
|
|
|-
| [[KS 1947+300]]
| HMXB
|
| 18.7
|
|
|
|-
| [[MAXI J0655-013]]
| HMXB
|
| 1129.1
|
|
|
|-
| [[MAXI J0903-531]]
| HMXB
|
| 14.05
|
|
|
|-
| [[MAXI J0911-655]]
| LMXB
|
| 0.00294
|
|
|
|-
| [[MAXI J1409-619]]
| HMXB
|
| 503.0
|
|
|
|-
| [[MAXI J1816-195]]
| LMXB
|
| 0.0018917896329928112
|
|
|
|-
| [[MXB 0656-072]]
| HMXB
|
| 160.7
|
|
|
|-
| [[MXB 1659-29]]
| LMXB
|
| 0.00176
|
|
|
|-
| [[MXB 1730-335]]
| LMXB
|
| 0.0032679738562091504
|
|
|
|-
| [[OAO 1657-415]]
| HMXB
| Vicente
| 37.03
|
|
|
|-
| [[PSR B1259-63]]
| HMXB
|
| 0.05
|
|
|
|-
| [[PSR J1023+0038]]
| LMXB
|
| 0.001687
|
|
|
|-
| [[PSR J1723-2837]]
| LMXB
|
| 0.00186219739292365
|
|
|
|-
| [[SAX J1324.4-6200]]
| HMXB
|
| 172.84
|
|
|
|-
| [[SAX J1748.9-2021]]
| LMXB
|
| 0.00226
|
|
|
|-
| [[SAX J1808.4-3658]]
| LMXB
|
| 0.00249
|
|
|
|-
| [[SAX J2103.5+4545]]
| HMXB
|
| 358.61
|
|
|
|-
| [[SGR 0755-2933]]
| HMXB
|
| 308.0
|
|
|
|-
| [[SRGA J124404.1-632232]]
| HMXB
| Aafia
| 538.7
|
|
|
|-
| [[SRGE J204319.0+443820]]
| HMXB
|
| 741.8
|
|
|
|-
| [[SWIFT J1749.4-2807]]
| LMXB
|
| 0.00193
|
|
|
|-
| [[SWIFT J1756.9-2508]]
| LMXB
|
| 0.005493
|
|
|
|-
| [[SWIFT J1843.5-0343]]
| LMXB
|
| 42.5
|
|
|
|-
| [[Sct X-1]]
| HMXB
|
| 112.0
|
|
|
|-
| [[Swift J0243.6+6124]]
| HMXB
|
| 9.87
|
|
|
|-
| [[Swift J0840.7-3516]]
| LMXB
|
| 8.96
|
|
|
|-
| [[Swift J1626.6-5156]]
| HMXB
|
| 15.36
|
|
|
|-
| [[Swift J1816.7-1613]]
| HMXB
|
| 143.69
|
|
|
|-
| [[V0332+53]]
| HMXB
|
| 4.4
|
|
|
|-
| [[XMM J174457-2850.3]]
| LMXB
|
| 5.2521
|
|
|
|-
| [[XSS J12270-4859]]
| LMXB
|
| 0.001686
|
|
|
|-
| [[XTE J1739-285]]
| LMXB
|
| 0.00258732212160414
|
|
|
|-
| [[XTE J1748-361]]
| LMXB
|
| 0.0018867924528301887
|
|
|
|-
| [[XTE J1829-098]]
| HMXB
|
| 7.85
|
|
|
|-
| [[XTE J1858+034]]
| HMXB
|
| 221.0
|
|
|
|-
| [[XTE J1859+083]]
| HMXB
|
| 9.79
|
|
|
|-
| [[XTE J1946+274]]
| HMXB
|
| 15.8
|
|
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-14T14:56:33Z

Zainab: /* Updated list of accreting X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars (pulse profile extractions) =

This is a list to organize a library of pulse profiles for many of the known accreting X-ray pulsars. For this we scanned the NuSTAR archive at [https://heasarc.gsfc.nasa.gov/docs/archive.html Heasarc] for all objects that are listed in the two [http://astro.uni-tuebingen.de/~xrbcat/ XRB catalogues]. All public obsids are downloaded to `/userdata/data/stierhof/pp-class/<object_name>/<obsid>`. This is more than 350 observations! After reprocessing (this creates a folder `reprocessed` in each obsid folder) the region files have to be created. Right now we are not interested in detailed analysis and for bright outbursts the region choice is not that important. If you want to contribute, please create '''one''' region file for the source and '''one''' for the background. The source should be a circle centered around the brightest part of the image. The background should be an annulus with inner radius as large as the source region, and the outer as large as possible. The source and background region files should be stored in the `reprocessed` folder as `src.reg` and `bkg.reg`. '''Note:''' The regions must be valid for both detector modules!

Once the region files are created it is straight forward to automatically extract all dataset. So please don't change anything else in the folder just yet. You can check the table if the data has been prepared (that is, if the `reprocessed` folder exists) and add the region files. If you do, please indicate it in the corresponding line in the table (searching for the source name should be helpful here).

Once we have all region files collected we can extract the pulse profiles!

{| class=wikitable
! Source
! Class
! Assignee
! Pulse Period
! Has Region
! Is Prepared
! Is Processed
|-
| [[1A 0535+262]]
| HMXB
|
| 103.47
|
|
|
|-
| [[1E 1145.1-6141]]
| HMXB
| Vicente
| 298.0
|
|
|
|-
| [[2RXP J130159.6-635806]]
| HMXB
|
| 643.0
|
|
|
|-
| [[2S 0114+650]]
| HMXB
|
| 10008.0
|
|
|
|-
| [[2S 1417-624]]
| HMXB
|
| 17.6
|
|
|
|-
| [[2S 1553-542]]
| HMXB
|
| 9.28
|
|
|
|-
| [[2S 1845-024]]
| HMXB
|
| 94.72
|
|
|
|-
| [[3A 1822-371]]
| LMXB
|
| 0.59
|
|
|
|-
| [[3U 1223-62]]
| HMXB
|
| 696.0
|
|
|
|-
| [[3U 1258-61]]
| HMXB
|
| 272.0
|
|
|
|-
| [[4U 0115+63]]
| HMXB
|
| 3.61
|
|
|
|-
| [[4U 0352+309]]
| HMXB
|
| 837.67
|
|
|
|-
| [[4U 0614+09]]
| LMXB
|
| 0.0020964360587002098
|
|
|
|-
| [[4U 1538-52]]
| HMXB
| Aafia
| 526.42
|
|
|
|-
| [[4U 1608-52]]
| LMXB
|
| 0.0016
|
|
|
|-
| [[4U 1626-67]]
| LMXB
|
| 7.7
|
|
|
|-
| [[4U 1636-536]]
| LMXB
|
| 0.001721
|
|
|
|-
| [[4U 1702-429]]
| LMXB
|
| 0.00303
|
|
|
|-
| [[4U 1728-34]]
| LMXB
|
| 0.0027548209366391185
|
|
|
|-
| [[4U 1901+03]]
| HMXB
|
| 2.76
|
|
|
|-
| [[4U 1907+09]]
| HMXB
| Aafia
| 438.0
|
|
|
|-
| [[4U 1909+07]]
| HMXB
| Aafia
| 603.6
|
|
|
|-
| [[4U 1915-05]]
| LMXB
|
| 0.0037
|
|
|
|-
| [[4U 1954+31]]
| HMXB
|
| 19400.0
|
|
|
|-
| [[4U 2206+54]]
| HMXB
|
| 5555.0
|
|
|
|-
| [[Aql X-1]]
| LMXB
|
| 0.00182
|
|
|
|-
| [[BSD 24-491]]
| HMXB
|
| 202.5
|
|
|
|-
| [[CXOGlb J174852.7-202124]]
| LMXB
|
| 0.004857
|
|
|
|-
| [[Cen X-3]]
| HMXB
|
| 4.8
|
|
|
|-
| [[Cep X-4]]
| HMXB
|
| 65.35
|
|
|
|-
| [[EXO 0748-676]]
| LMXB
|
| 0.0019157088122605363
|
|
|
|-
| [[EXO 2030+375]]
| HMXB
|
| 41.31
|
|
|
|-
| [[GRO J1008-57]]
| HMXB
| Aafia
| 93.5
|
|
|
|-
| [[GRO J1744-28]]
| LMXB
|
| 0.467
|
|
|
|-
| [[GRO J1750-27]]
| HMXB
|
| 4.45
|
|
|
|-
| [[GRO J2058+42]]
| HMXB
|
| 195.25
|
|
|
|-
| [[GRS 1741.9-2853]]
| LMXB
|
| 0.001697792869269949
|
|
|
|-
| [[GX 1+4]]
| LMXB
|
| 138.17
|
|
|
|-
| [[Ginga 0834-430]]
| HMXB
|
| 12.3
|
|
|
|-
| [[HD 110432]]
| HMXB
|
| 14200.0
|
|
|
|-
| [[HD 77581]]
| HMXB
|
| 283.0
|
|
|
|-
| [[Her X-1]]
| LMXB
|
| 1.24
|
|
|
|-
| [[IGR J00291+5934]]
| LMXB
|
| 0.00167
|
|
|
|-
| [[IGR J06074+2205]]
| HMXB
|
| 373.2
|
|
|
|-
| [[IGR J11215-5952]]
| HMXB
|
| 186.8
|
|
|
|-
| [[IGR J16320-4751]]
| HMXB
|
| 1308.8
|
|
|
|-
| [[IGR J16358-4726]]
| LMXB
|
| 5880.0
|
|
|
|-
| [[IGR J16393-4643]]
| HMXB
| Aafia
| 908.79
|
|
|
|-
| [[IGR J16418-4532]]
| HMXB
| Aafia
| 1246.0
|
|
|
|-
| [[IGR J16493-4348]]
| HMXB
|
| 1093.1
|
|
|
|-
| [[IGR J16597-3704]]
| LMXB
|
| 0.00951
|
|
|
|-
| [[IGR J17062-6143]]
| LMXB
| Vicente
| 0.00611
|
|
|
|-
| [[IGR J17329-2731]]
| LMXB
|
| 6680.0
|
|
|
|-
| [[IGR J17379-3747]]
| LMXB
| Vicente
| 0.002136
|
|
|
|-
| [[IGR J17480-2446]]
| LMXB
|
| 0.09054
|
|
|
|-
| [[IGR J17494-3030]]
| LMXB
|
| 0.002659219644588837
|
|
|
|-
| [[IGR J17498-2921]]
| LMXB
|
| 0.002494
|
|
|
|-
| [[IGR J17511-3057]]
| LMXB
|
| 0.00408
|
|
|
|-
| [[IGR J17544-2619]]
| HMXB
|
| 71.49
|
|
|
|-
| [[IGR J17591-2342]]
| LMXB
|
| 0.001897
|
|
|
|-
| [[IGR J18027-2016]]
| HMXB
|
| 139.6
|
|
|
|-
| [[IGR J18219-1347]]
| HMXB
|
| 52.46
|
|
|
|-
| [[IGR J18245-2452]]
| LMXB
|
| 0.00393
|
|
|
|-
| [[IGR J19294+1816]]
| HMXB
|
| 12.44
|
|
|
|-
| [[IGR J21343+4738]]
| HMXB
|
| 322.7
|
|
|
|-
| [[KS 1947+300]]
| HMXB
|
| 18.7
|
|
|
|-
| [[MAXI J0655-013]]
| HMXB
|
| 1129.1
|
|
|
|-
| [[MAXI J0903-531]]
| HMXB
|
| 14.05
|
|
|
|-
| [[MAXI J0911-655]]
| LMXB
|
| 0.00294
|
|
|
|-
| [[MAXI J1409-619]]
| HMXB
|
| 503.0
|
|
|
|-
| [[MAXI J1816-195]]
| LMXB
|
| 0.0018917896329928112
|
|
|
|-
| [[MXB 0656-072]]
| HMXB
|
| 160.7
|
|
|
|-
| [[MXB 1659-29]]
| LMXB
|
| 0.00176
|
|
|
|-
| [[MXB 1730-335]]
| LMXB
|
| 0.0032679738562091504
|
|
|
|-
| [[OAO 1657-415]]
| HMXB
| Vicente
| 37.03
|
|
|
|-
| [[PSR B1259-63]]
| HMXB
|
| 0.05
|
|
|
|-
| [[PSR J1023+0038]]
| LMXB
|
| 0.001687
|
|
|
|-
| [[PSR J1723-2837]]
| LMXB
|
| 0.00186219739292365
|
|
|
|-
| [[SAX J1324.4-6200]]
| HMXB
|
| 172.84
|
|
|
|-
| [[SAX J1748.9-2021]]
| LMXB
|
| 0.00226
|
|
|
|-
| [[SAX J1808.4-3658]]
| LMXB
|
| 0.00249
|
|
|
|-
| [[SAX J2103.5+4545]]
| HMXB
|
| 358.61
|
|
|
|-
| [[SGR 0755-2933]]
| HMXB
|
| 308.0
|
|
|
|-
| [[SRGA J124404.1-632232]]
| HMXB
|
| 538.7
|
|
|
|-
| [[SRGE J204319.0+443820]]
| HMXB
|
| 741.8
|
|
|
|-
| [[SWIFT J1749.4-2807]]
| LMXB
|
| 0.00193
|
|
|
|-
| [[SWIFT J1756.9-2508]]
| LMXB
|
| 0.005493
|
|
|
|-
| [[SWIFT J1843.5-0343]]
| LMXB
|
| 42.5
|
|
|
|-
| [[Sct X-1]]
| HMXB
|
| 112.0
|
|
|
|-
| [[Swift J0243.6+6124]]
| HMXB
|
| 9.87
|
|
|
|-
| [[Swift J0840.7-3516]]
| LMXB
|
| 8.96
|
|
|
|-
| [[Swift J1626.6-5156]]
| HMXB
|
| 15.36
|
|
|
|-
| [[Swift J1816.7-1613]]
| HMXB
|
| 143.69
|
|
|
|-
| [[V0332+53]]
| HMXB
|
| 4.4
|
|
|
|-
| [[XMM J174457-2850.3]]
| LMXB
|
| 5.2521
|
|
|
|-
| [[XSS J12270-4859]]
| LMXB
|
| 0.001686
|
|
|
|-
| [[XTE J1739-285]]
| LMXB
|
| 0.00258732212160414
|
|
|
|-
| [[XTE J1748-361]]
| LMXB
|
| 0.0018867924528301887
|
|
|
|-
| [[XTE J1829-098]]
| HMXB
|
| 7.85
|
|
|
|-
| [[XTE J1858+034]]
| HMXB
|
| 221.0
|
|
|
|-
| [[XTE J1859+083]]
| HMXB
|
| 9.79
|
|
|
|-
| [[XTE J1946+274]]
| HMXB
|
| 15.8
|
|
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-14T14:49:55Z

Zainab: /* Updated list of accreting X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars (pulse profile extractions) =

This is a list to organize a library of pulse profiles for many of the known accreting X-ray pulsars. For this we scanned the NuSTAR archive at [https://heasarc.gsfc.nasa.gov/docs/archive.html Heasarc] for all objects that are listed in the two [http://astro.uni-tuebingen.de/~xrbcat/ XRB catalogues]. All public obsids are downloaded to `/userdata/data/stierhof/pp-class/<object_name>/<obsid>`. This is more than 350 observations! After reprocessing (this creates a folder `reprocessed` in each obsid folder) the region files have to be created. Right now we are not interested in detailed analysis and for bright outbursts the region choice is not that important. If you want to contribute, please create '''one''' region file for the source and '''one''' for the background. The source should be a circle centered around the brightest part of the image. The background should be an annulus with inner radius as large as the source region, and the outer as large as possible. The source and background region files should be stored in the `reprocessed` folder as `src.reg` and `bkg.reg`. '''Note:''' The regions must be valid for both detector modules!

Once the region files are created it is straight forward to automatically extract all dataset. So please don't change anything else in the folder just yet. You can check the table if the data has been prepared (that is, if the `reprocessed` folder exists) and add the region files. If you do, please indicate it in the corresponding line in the table (searching for the source name should be helpful here).

Once we have all region files collected we can extract the pulse profiles!

{| class=wikitable
! Source
! Class
! Assignee
! Pulse Period
! Has Region
! Is Prepared
! Is Processed
|-
| [[1A 0535+262]]
| HMXB
|
| 103.47
|
|
|
|-
| [[1E 1145.1-6141]]
| HMXB
|
| 298.0
|
|
|
|-
| [[2RXP J130159.6-635806]]
| HMXB
|
| 643.0
|
|
|
|-
| [[2S 0114+650]]
| HMXB
|
| 10008.0
|
|
|
|-
| [[2S 1417-624]]
| HMXB
|
| 17.6
|
|
|
|-
| [[2S 1553-542]]
| HMXB
|
| 9.28
|
|
|
|-
| [[2S 1845-024]]
| HMXB
| Aafia
| 94.72
|
|
|
|-
| [[3A 1822-371]]
| LMXB
|
| 0.59
|
|
|
|-
| [[3U 1223-62]]
| HMXB
|
| 696.0
|
|
|
|-
| [[3U 1258-61]]
| HMXB
|
| 272.0
|
|
|
|-
| [[4U 0115+63]]
| HMXB
|
| 3.61
|
|
|
|-
| [[4U 0352+309]]
| HMXB
|
| 837.67
|
|
|
|-
| [[4U 0614+09]]
| LMXB
|
| 0.0020964360587002098
|
|
|
|-
| [[4U 1538-52]]
| HMXB
|
| 526.42
|
|
|
|-
| [[4U 1608-52]]
| LMXB
|
| 0.0016
|
|
|
|-
| [[4U 1626-67]]
| LMXB
|
| 7.7
|
|
|
|-
| [[4U 1636-536]]
| LMXB
|
| 0.001721
|
|
|
|-
| [[4U 1702-429]]
| LMXB
|
| 0.00303
|
|
|
|-
| [[4U 1728-34]]
| LMXB
|
| 0.0027548209366391185
|
|
|
|-
| [[4U 1901+03]]
| HMXB
|
| 2.76
|
|
|
|-
| [[4U 1907+09]]
| HMXB
|
| 438.0
|
|
|
|-
| [[4U 1909+07]]
| HMXB
| Aafia
| 603.6
|
|
|
|-
| [[4U 1915-05]]
| LMXB
|
| 0.0037
|
|
|
|-
| [[4U 1954+31]]
| HMXB
|
| 19400.0
|
|
|
|-
| [[4U 2206+54]]
| HMXB
|
| 5555.0
|
|
|
|-
| [[Aql X-1]]
| LMXB
|
| 0.00182
|
|
|
|-
| [[BSD 24-491]]
| HMXB
|
| 202.5
|
|
|
|-
| [[CXOGlb J174852.7-202124]]
| LMXB
|
| 0.004857
|
|
|
|-
| [[Cen X-3]]
| HMXB
|
| 4.8
|
|
|
|-
| [[Cep X-4]]
| HMXB
|
| 65.35
|
|
|
|-
| [[EXO 0748-676]]
| LMXB
|
| 0.0019157088122605363
|
|
|
|-
| [[EXO 2030+375]]
| HMXB
| Aafia
| 41.31
|
|
|
|-
| [[GRO J1008-57]]
| HMXB
| Aafia
| 93.5
|
|
|
|-
| [[GRO J1744-28]]
| LMXB
|
| 0.467
|
|
|
|-
| [[GRO J1750-27]]
| HMXB
|
| 4.45
|
|
|
|-
| [[GRO J2058+42]]
| HMXB
|
| 195.25
|
|
|
|-
| [[GRS 1741.9-2853]]
| LMXB
|
| 0.001697792869269949
|
|
|
|-
| [[GX 1+4]]
| LMXB
|
| 138.17
|
|
|
|-
| [[Ginga 0834-430]]
| HMXB
|
| 12.3
|
|
|
|-
| [[HD 110432]]
| HMXB
|
| 14200.0
|
|
|
|-
| [[HD 77581]]
| HMXB
|
| 283.0
|
|
|
|-
| [[Her X-1]]
| LMXB
|
| 1.24
|
|
|
|-
| [[IGR J00291+5934]]
| LMXB
|
| 0.00167
|
|
|
|-
| [[IGR J06074+2205]]
| HMXB
|
| 373.2
|
|
|
|-
| [[IGR J11215-5952]]
| HMXB
| Aafia
| 186.8
|
|
|
|-
| [[IGR J16320-4751]]
| HMXB
|
| 1308.8
|
|
|
|-
| [[IGR J16358-4726]]
| LMXB
|
| 5880.0
|
|
|
|-
| [[IGR J16393-4643]]
| HMXB
|
| 908.79
|
|
|
|-
| [[IGR J16418-4532]]
| HMXB
| Vicente
| 1246.0
|
|
|
|-
| [[IGR J16493-4348]]
| HMXB
|
| 1093.1
|
|
|
|-
| [[IGR J16597-3704]]
| LMXB
|
| 0.00951
|
|
|
|-
| [[IGR J17062-6143]]
| LMXB
| Vicente
| 0.00611
|
|
|
|-
| [[IGR J17329-2731]]
| LMXB
|
| 6680.0
|
|
|
|-
| [[IGR J17379-3747]]
| LMXB
| Vicente
| 0.002136
|
|
|
|-
| [[IGR J17480-2446]]
| LMXB
|
| 0.09054
|
|
|
|-
| [[IGR J17494-3030]]
| LMXB
|
| 0.002659219644588837
|
|
|
|-
| [[IGR J17498-2921]]
| LMXB
|
| 0.002494
|
|
|
|-
| [[IGR J17511-3057]]
| LMXB
|
| 0.00408
|
|
|
|-
| [[IGR J17544-2619]]
| HMXB
|
| 71.49
|
|
|
|-
| [[IGR J17591-2342]]
| LMXB
|
| 0.001897
|
|
|
|-
| [[IGR J18027-2016]]
| HMXB
|
| 139.6
|
|
|
|-
| [[IGR J18219-1347]]
| HMXB
|
| 52.46
|
|
|
|-
| [[IGR J18245-2452]]
| LMXB
|
| 0.00393
|
|
|
|-
| [[IGR J19294+1816]]
| HMXB
|
| 12.44
|
|
|
|-
| [[IGR J21343+4738]]
| HMXB
|
| 322.7
|
|
|
|-
| [[KS 1947+300]]
| HMXB
|
| 18.7
|
|
|
|-
| [[MAXI J0655-013]]
| HMXB
|
| 1129.1
|
|
|
|-
| [[MAXI J0903-531]]
| HMXB
|
| 14.05
|
|
|
|-
| [[MAXI J0911-655]]
| LMXB
|
| 0.00294
|
|
|
|-
| [[MAXI J1409-619]]
| HMXB
|
| 503.0
|
|
|
|-
| [[MAXI J1816-195]]
| LMXB
|
| 0.0018917896329928112
|
|
|
|-
| [[MXB 0656-072]]
| HMXB
|
| 160.7
|
|
|
|-
| [[MXB 1659-29]]
| LMXB
|
| 0.00176
|
|
|
|-
| [[MXB 1730-335]]
| LMXB
|
| 0.0032679738562091504
|
|
|
|-
| [[OAO 1657-415]]
| HMXB
|
| 37.03
|
|
|
|-
| [[PSR B1259-63]]
| HMXB
|
| 0.05
|
|
|
|-
| [[PSR J1023+0038]]
| LMXB
|
| 0.001687
|
|
|
|-
| [[PSR J1723-2837]]
| LMXB
|
| 0.00186219739292365
|
|
|
|-
| [[SAX J1324.4-6200]]
| HMXB
|
| 172.84
|
|
|
|-
| [[SAX J1748.9-2021]]
| LMXB
|
| 0.00226
|
|
|
|-
| [[SAX J1808.4-3658]]
| LMXB
|
| 0.00249
|
|
|
|-
| [[SAX J2103.5+4545]]
| HMXB
| Aafia
| 358.61
|
|
|
|-
| [[SGR 0755-2933]]
| HMXB
|
| 308.0
|
|
|
|-
| [[SRGA J124404.1-632232]]
| HMXB
|
| 538.7
|
|
|
|-
| [[SRGE J204319.0+443820]]
| HMXB
|
| 741.8
|
|
|
|-
| [[SWIFT J1749.4-2807]]
| LMXB
|
| 0.00193
|
|
|
|-
| [[SWIFT J1756.9-2508]]
| LMXB
|
| 0.005493
|
|
|
|-
| [[SWIFT J1843.5-0343]]
| LMXB
|
| 42.5
|
|
|
|-
| [[Sct X-1]]
| HMXB
|
| 112.0
|
|
|
|-
| [[Swift J0243.6+6124]]
| HMXB
|
| 9.87
|
|
|
|-
| [[Swift J0840.7-3516]]
| LMXB
|
| 8.96
|
|
|
|-
| [[Swift J1626.6-5156]]
| HMXB
|
| 15.36
|
|
|
|-
| [[Swift J1816.7-1613]]
| HMXB
|
| 143.69
|
|
|
|-
| [[V0332+53]]
| HMXB
|
| 4.4
|
|
|
|-
| [[XMM J174457-2850.3]]
| LMXB
|
| 5.2521
|
|
|
|-
| [[XSS J12270-4859]]
| LMXB
|
| 0.001686
|
|
|
|-
| [[XTE J1739-285]]
| LMXB
|
| 0.00258732212160414
|
|
|
|-
| [[XTE J1748-361]]
| LMXB
|
| 0.0018867924528301887
|
|
|
|-
| [[XTE J1829-098]]
| HMXB
|
| 7.85
|
|
|
|-
| [[XTE J1858+034]]
| HMXB
|
| 221.0
|
|
|
|-
| [[XTE J1859+083]]
| HMXB
|
| 9.79
|
|
|
|-
| [[XTE J1946+274]]
| HMXB
|
| 15.8
|
|
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-14T00:36:58Z

Zainab: /* Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars (pulse profile extractions) =

This is a list to organize a library of pulse profiles for many of the known accreting X-ray pulsars. For this we scanned the NuSTAR archive at [https://heasarc.gsfc.nasa.gov/docs/archive.html Heasarc] for all objects that are listed in the two [http://astro.uni-tuebingen.de/~xrbcat/ XRB catalogues]. All public obsids are downloaded to `/userdata/data/stierhof/pp-class/<object_name>/<obsid>`. This is more than 350 observations! After reprocessing (this creates a folder `reprocessed` in each obsid folder) the region files have to be created. Right now we are not interested in detailed analysis and for bright outbursts the region choice is not that important. If you want to contribute, please create '''one''' region file for the source and '''one''' for the background. The source should be a circle centered around the brightest part of the image. The background should be an annulus with inner radius as large as the source region, and the outer as large as possible. The source and background region files should be stored in the `reprocessed` folder as `src.reg` and `bkg.reg`. '''Note:''' The regions must be valid for both detector modules!

Once the region files are created it is straight forward to automatically extract all dataset. So please don't change anything else in the folder just yet. You can check the table if the data has been prepared (that is, if the `reprocessed` folder exists) and add the region files. If you do, please indicate it in the corresponding line in the table (searching for the source name should be helpful here).

Once we have all region files collected we can extract the pulse profiles!

{| class=wikitable
! Source
! Assignee
! Pulse Period
! Is Prepared
! Has Region
! Is Processed
|-
| [[IGR J00370+6122]]
|
| 674.0
|
|
|
|-
| [[2S 0114+650]]
|
| 10008.0
|
|
|
|-
| [[4U 0115+63]]
|
| 3.61
|
|
|
|-
| [[RX J0146.9+6121]]
| Aafia
| 1407.4
|
|
|
|-
| [[IGR J01583+6713]]
|
| 469.2
|
|
|
|-
| [[Swift J0243.6+6124]]
|
| 9.87
|
|
|
|-
| [[V0332+53]]
|
| 4.4
|
|
|
|-
| [[4U 0352+309]]
|
| 837.67
|
|
|
|-
| [[BSD 24-491]]
|
| 202.5
|
|
|
|-
| [[1A 0535+262]]
|
| 103.47
|
|
|
|-
| [[IGR J06074+2205]]
|
| 373.2
|
|
|
|-
| [[PSR J0635+0533]]
|
| 0.03
|
|
|
|-
| [[MAXI J0655-013]]
|
| 1129.1
|
|
|
|-
| [[MXB 0656-072]]
|
| 160.7
|
|
|
|-
| [[4U 0728-25]]
|
| 103.14
|
|
|
|-
| [[SGR 0755-2933]]
|
| 308.0
|
|
|
|-
| [[LS 992]]
|
| 31.91
|
|
|
|-
| [[Ginga 0834-430]]
|
| 12.3
|
|
|
|-
| [[HD 77581]]
|
| 283.0
|
|
|
|-
| [[MAXI J0903-531]]
|
| 14.05
|
|
|
|-
| [[GRO J1008-57]]
| Aafia
| 93.5
|
|
|
|-
| [[LS 1698]]
|
| 862.0
|
|
|
|-
| [[1A 1118-61]]
|
| 405.0
|
|
|
|-
| [[Cen X-3]]
|
| 4.8
|
|
|
|-
| [[IGR J11215-5952]]
| Aafia
| 186.8
|
|
|
|-
| [[IGR J11435-6109]]
| Aafia
| 161.8
|
|
|
|-
| [[1E 1145.1-6141]]
|
| 298.0
|
|
|
|-
| [[4U 1145-619]]
|
| 292.4
|
|
|
|-
| [[3U 1223-62]]
|
| 696.0
|
|
|
|-
| [[1A 1238-59]]
|
| 191.0
|
|
|
|-
| [[HD 110432]]
|
| 14200.0
|
|
|
|-
| [[SRGA J124404.1-632232]]
|
| 538.7
|
|
|
|-
| [[3U 1258-61]]
|
| 272.0
|
|
|
|-
| [[2RXP J130159.6-635806]]
|
| 643.0
|
|
|
|-
| [[PSR B1259-63]]
|
| 0.05
|
|
|
|-
| [[SAX J1324.4-6200]]
|
| 172.84
|
|
|
|-
| [[HD 119682]]
|
| 1500.0
|
|
|
|-
| [[MAXI J1409-619]]
|
| 503.0
|
|
|
|-
| [[2S 1417-624]]
|
| 17.6
|
|
|
|-
| [[IGR J14488-5942]]
|
| 33.42
|
|
|
|-
| [[4U 1538-52]]
|
| 526.42
|
|
|
|-
| [[XTE J1543-568]]
|
| 27.12
|
|
|
|-
| [[2S 1553-542]]
|
| 9.28
|
|
|
|-
| [[Swift J1626.6-5156]]
|
| 15.36
|
|
|
|-
| [[IGR J16320-4751]]
|
| 1308.8
|
|
|
|-
| [[IGR J16393-4643]]
|
| 908.79
|
|
|
|-
| [[IGR J16418-4532]]
| Vicente
| 1246.0
|
|
|
|-
| [[IGR J16465-4507]]
|
| 228.0
|
|
|
|-
| [[IGR J16493-4348]]
|
| 1093.1
|
|
|
|-
| [[AX J1700.2-4220]]
|
| 54.2
|
|
|
|-
| [[OAO 1657-415]]
|
| 37.03
|
|
|
|-
| [[IGR J17200-3116]]
|
| 328.2
|
|
|
|-
| [[IGR J17252-3616]]
|
| 413.7
|
|
|
|-
| [[HD 161103]]
| Aafia
| 3245.0
|
|
|
|-
| [[AX J1749.1-2733]]
|
| 132.0
|
|
|
|-
| [[AX J1749.2-2725]]
|
| 220.38
|
|
|
|-
| [[GRO J1750-27]]
|
| 4.45
|
|
|
|-
| [[IGR J17544-2619]]
|
| 71.49
|
|
|
|-
| [[IGR J18027-2016]]
|
| 139.6
|
|
|
|-
| [[Swift J1816.7-1613]]
|
| 143.69
|
|
|
|-
| [[IGR J18179-1621]]
|
| 11.82
|
|
|
|-
| [[AX J1820.5-1434]]
| Vicente
| 152.3
|
|
|
|-
| [[IGR J18219-1347]]
|
| 52.46
|
|
|
|-
| [[XTE J1824-141]]
|
| 120.0
|
|
|
|-
| [[XTE J1829-098]]
|
| 7.85
|
|
|
|-
| [[Sct X-1]]
|
| 112.0
|
|
|
|-
| [[Ginga 1839-04]]
|
| 81.1
|
|
|
|-
| [[Ginga 1843+009]]
|
| 29.48
|
|
|
|-
| [[IGR J18462-0223]]
|
| 997.0
|
|
|
|-
| [[2S 1845-024]]
| Aafia
| 94.72
|
|
|
|-
| [[IGR J18483-0311]]
|
| 21.05
|
|
|
|-
| [[XTE J1855-026]]
|
| 361.0
|
|
|
|-
| [[XTE J1858+034]]
|
| 221.0
|
|
|
|-
| [[XTE J1859+083]]
|
| 9.79
|
|
|
|-
| [[4U 1901+03]]
|
| 2.76
|
|
|
|-
| [[XTE J1906+090]]
|
| 89.17
|
|
|
|-
| [[4U 1907+09]]
|
| 438.0
|
|
|
|-
| [[AX J1910.7+0917]]
|
| 36200.0
|
|
|
|-
| [[4U 1909+07]]
| Aafia
| 603.6
|
|
|
|-
| [[IGR J19140+0951]]
|
| 5937.0
|
|
|
|-
| [[IGR J19294+1816]]
|
| 12.44
|
|
|
|-
| [[XTE J1946+274]]
|
| 15.8
|
|
|
|-
| [[KS 1947+300]]
|
| 18.7
|
|
|
|-
| [[4U 1954+31]]
|
| 19400.0
|
|
|
|-
| [[2MASS J20002185+3211232]]
|
| 890.0
|
|
|
|-
| [[W63 X-1]]
|
| 36.0
|
|
|
|-
| [[EXO 2030+375]]
| Aafia
| 41.31
|
|
|
|-
| [[SRGE J204319.0+443820]]
|
| 741.8
|
|
|
|-
| [[GRO J2058+42]]
|
| 195.25
|
|
|
|-
| [[SAX J2103.5+4545]]
| Aafia
| 358.61
|
|
|
|-
| [[IGR J21343+4738]]
|
| 322.7
|
|
|
|-
| [[Cep X-4]]
|
| 65.35
|
|
|
|-
| [[4U 2206+54]]
|
| 5555.0
|
|
|
|-
| [[SAX J2239.3+6116]]
|
| 1247.0
|
|
|
|-
| [[IGR J22534+6243]]
|
| 46.75
|
|
|
|-
| [[IGR J00291+5934]]
|
| 0.00167
|
|
|
|-
| [[4U 0614+09]]
|
| 0.0020964360587002098
|
|
|
|-
| [[EXO 0748-676]]
|
| 0.0019157088122605363
|
|
|
|-
| [[Swift J0840.7-3516]]
|
| 8.96
|
|
|
|-
| [[MAXI J0911-655]]
|
| 0.00294
|
|
|
|-
| [[XTE J0929-314]]
|
| 0.0054
|
|
|
|-
| [[PSR J1023+0038]]
|
| 0.001687
|
|
|
|-
| [[XSS J12270-4859]]
|
| 0.001686
|
|
|
|-
| [[1FGL J1417.7-4407]]
|
| 0.00266
|
|
|
|-
| [[SAX J1452.8-5949]]
|
| 437.4
|
|
|
|-
| [[4U 1608-52]]
|
| 0.0016
|
|
|
|-
| [[4U 1626-67]]
|
| 7.7
|
|
|
|-
| [[IGR J16358-4726]]
|
| 5880.0
|
|
|
|-
| [[4U 1636-536]]
|
| 0.001721
|
|
|
|-
| [[Her X-1]]
|
| 1.24
|
|
|
|-
| [[IGR J16597-3704]]
|
| 0.00951
|
|
|
|-
| [[MXB 1659-29]]
|
| 0.00176
|
|
|
|-
| [[4U 1702-429]]
|
| 0.00303
|
|
|
|-
| [[IGR J17062-6143]]
|
| 0.00611
|
|
|
|-
| [[IGR J17191-2821]]
|
| 0.003389830508474576
|
|
|
|-
| [[PSR J1723-2837]]
|
| 0.00186219739292365
|
|
|
|-
| [[4U 1728-34]]
|
| 0.0027548209366391185
|
|
|
|-
| [[GX 1+4]]
|
| 138.17
|
|
|
|-
| [[IGR J17329-2731]]
|
| 6680.0
|
|
|
|-
| [[MXB 1730-335]]
|
| 0.0032679738562091504
|
|
|
|-
| [[KS 1731-260]]
|
| 0.0019
|
|
|
|-
| [[IGR J17379-3747]]
|
| 0.002136
|
|
|
|-
| [[XTE J1739-285]]
|
| 0.00258732212160414
|
|
|
|-
| [[GRO J1744-28]]
|
| 0.467
|
|
|
|-
| [[XMM J174457-2850.3]]
|
| 5.2521
|
|
|
|-
| [[GRS 1741.9-2853]]
|
| 0.001697792869269949
|
|
|
|-
| [[IGR J17480-2446]]
|
| 0.09054
|
|
|
|-
| [[XTE J1748-361]]
|
| 0.0018867924528301887
|
|
|
|-
| [[SAX J1748.9-2021]]
|
| 0.00226
|
|
|
|-
| [[CXOGlb J174852.7-202124]]
|
| 0.004857
|
|
|
|-
| [[IGR J17494-3030]]
|
| 0.002659219644588837
|
|
|
|-
| [[SWIFT J1749.4-2807]]
|
| 0.00193
|
|
|
|-
| [[IGR J17498-2921]]
|
| 0.002494
|
|
|
|-
| [[SAX J1750.8-2900]]
|
| 0.0017
|
|
|
|-
| [[IGR J17511-3057]]
|
| 0.00408
|
|
|
|-
| [[XTE J1751-305]]
|
| 0.0023
|
|
|
|-
| [[SWIFT J1756.9-2508]]
|
| 0.005493
|
|
|
|-
| [[IGR J17591-2342]]
|
| 0.001897
|
|
|
|-
| [[XTE J1807-294]]
|
| 0.00525
|
|
|
|-
| [[SAX J1808.4-3658]]
|
| 0.00249
|
|
|
|-
| [[4U 1807-10]]
|
| 4.45
|
|
|
|-
| [[XTE J1814-338]]
|
| 0.0032
|
|
|
|-
| [[MAXI J1816-195]]
|
| 0.0018917896329928112
|
|
|
|-
| [[3XMM J181923.7-170616]]
|
| 407.9
|
|
|
|-
| [[IGR J18245-2452]]
|
| 0.00393
|
|
|
|-
| [[3A 1822-371]]
|
| 0.59
|
|
|
|-
| [[SWIFT J1843.5-0343]]
|
| 42.5
|
|
|
|-
| [[HETE J1900.1-2455]]
|
| 0.00265
|
|
|
|-
| [[Aql X-1]]
|
| 0.00182
|
|
|
|-
| [[4U 1915-05]]
|
| 0.0037
|
|
|
|-
| [[MAXI J1957+032]]
|
| 0.0031883308062763114
|
|
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T16:15:47Z

Zainab: /* Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) =

{| class=wikitable
! Source
! Assignee
! Regions
! Pulse period
|-
| [[IGR J00370+6122]]
|
|
| 674.000000
|-
| [[2S 0114+650]]
|
|
| 10008.000000
|-
| [[4U 0115+63]]
|
|
| 3.610000
|-
| [[RX J0146.9+6121]]
|
|
| 1407.400000
|-
| [[IGR J01583+6713]]
|
|
| 469.200000
|-
| [[Swift J0243.6+6124]]
|
|
| 9.870000
|-
| [[V0332+53]]
|
|
| 4.400000
|-
| [[4U 0352+309]]
|
|
| 837.670000
|-
| [[BSD 24-491]]
|
|
| 202.500000
|-
| [[1A 0535+262]]
| Aafia
| Y
| 103.470000
|-
| [[IGR J06074+2205]]
|
|
| 373.200000
|-
| [[PSR J0635+0533]]
|
|
| 0.030000
|-
| [[MXB 0656-072]]
|
|
| 160.700000
|-
| [[4U 0728-25]]
|
|
| 103.140000
|-
| [[SGR 0755-2933]]
|
|
| 308.000000
|-
| [[LS 992]]
|
|
| 31.910000
|-
| [[Ginga 0834-430]]
|
|
| 12.300000
|-
| [[HD 77581]]
|
|
| 283.000000
|-
| [[MAXI J0903-531]]
|
|
| 14.050000
|-
| [[GRO J1008-57]]
| Aafia
| Y
| 93.500000
|-
| [[LS 1698]]
|
|
| 862.000000
|-
| [[1A 1118-61]]
|
|
| 405.000000
|-
| [[Cen X-3]]
|
|
| 4.800000
|-
| [[IGR J11215-5952]]
|
|
| 186.800000
|-
| [[IGR J11435-6109]]
|
|
| 161.800000
|-
| [[1E 1145.1-6141]]
| Vicente
| Y
| 298.000000
|-
| [[4U 1145-619]]
|
|
| 292.400000
|-
| [[3U 1223-62]]
|
|
| 696.000000
|-
| [[1A 1238-59]]
|
|
| 191.000000
|-
| [[HD 110432]]
|
|
| 14200.000000
|-
| [[SRGA J124404.1-632232]]
| Aafia
| Y
| 538.700000
|-
| [[3U 1258-61]]
| Aafia
| Y
| 272.000000
|-
| [[2RXP J130159.6-635806]]
|
|
| 643.000000
|-
| [[PSR B1259-63]]
|
|
| 0.050000
|-
| [[SAX J1324.4-6200]]
|
|
| 172.840000
|-
| [[HD 119682]]
|
|
| 1500.000000
|-
| [[MAXI J1409-619]]
|
|
| 503.000000
|-
| [[2S 1417-624]]
|
|
| 17.600000
|-
| [[IGR J14488-5942]]
|
|
| 33.420000
|-
| [[4U 1538-52]]
| Aafia
| Y
| 526.420000
|-
| [[XTE J1543-568]]
|
|
| 27.120000
|-
| [[2S 1553-542]]
|
|
| 9.280000
|-
| [[Swift J1626.6-5156]]
|
|
| 15.360000
|-
| [[IGR J16320-4751]]
|
|
| 1303.000000
|-
| [[IGR J16393-4643]]
| Aafia
| Y
| 908.790000
|-
| [[IGR J16418-4532]]
| Aafia
| Y
| 1246.000000
|-
| [[IGR J16465-4507]]
|
|
| 228.000000
|-
| [[IGR J16493-4348]]
|
|
| 1093.100000
|-
| [[AX J1700.2-4220]]
|
|
| 54.200000
|-
| [[OAO 1657-415]]
| Vicente
| Y
| 37.030000
|-
| [[IGR J17200-3116]]
|
|
| 328.200000
|-
| [[IGR J17252-3616]]
|
|
| 413.700000
|-
| [[HD 161103]]
|
|
| 3245.000000
|-
| [[AX J1749.1-2733]]
|
|
| 132.000000
|-
| [[AX J1749.2-2725]]
|
|
| 220.380000
|-
| [[GRO J1750-27]]
|
|
| 4.450000
|-
| [[IGR J17544-2619]]
|
|
| 71.490000
|-
| [[IGR J18027-2016]]
|
|
| 139.600000
|-
| [[Swift J1816.7-1613]]
|
|
| 143.690000
|-
| [[IGR J18179-1621]]
|
|
| 11.820000
|-
| [[AX J1820.5-1434]]
|
|
| 152.300000
|-
| [[IGR J18219-1347]]
|
|
| 52.460000
|-
| [[XTE J1824-141]]
|
|
| 120.000000
|-
| [[XTE J1829-098]]
|
|
| 7.850000
|-
| [[Sct X-1]]
|
|
| 112.000000
|-
| [[Ginga 1839-04]]
|
|
| 81.100000
|-
| [[Ginga 1843+009]]
|
|
| 29.480000
|-
| [[IGR J18462-0223]]
|
|
| 997.000000
|-
| [[2S 1845-024]]
|
|
| 94.720000
|-
| [[IGR J18483-0311]]
|
|
| 21.050000
|-
| [[XTE J1855-026]]
|
|
| 361.000000
|-
| [[XTE J1858+034]]
|
|
| 221.000000
|-
| [[XTE J1859+083]]
|
|
| 9.790000
|-
| [[4U 1901+03]]
| Aafia
| Y
| 2.760000
|-
| [[XTE J1906+090]]
|
|
| 89.170000
|-
| [[4U 1907+09]]
| Aafia
| Y
| 438.000000
|-
| [[AX J1910.7+0917]]
|
|
| 36200.000000
|-
| [[4U 1909+07]]
|
|
| 603.600000
|-
| [[IGR J19140+0951]]
|
|
| 5937.000000
|-
| [[IGR J19294+1816]]
|
|
| 12.440000
|-
| [[XTE J1946+274]]
|
|
| 15.800000
|-
| [[KS 1947+300]]
|
|
| 18.700000
|-
| [[4U 1954+31]]
|
|
| 19400.000000
|-
| [[2MASS J20002185+3211232]]
|
|
| 890.000000
|-
| [[W63 X-1]]
|
|
| 36.000000
|-
| [[EXO 2030+375]]
|
|
| 41.310000
|-
| [[SRGE J204319.0+443820]]
|
|
| 741.800000
|-
| [[GRO J2058+42]]
|
|
| 195.250000
|-
| [[SAX J2103.5+4545]]
|
|
| 358.610000
|-
| [[IGR J21343+4738]]
|
|
| 322.700000
|-
| [[Cep X-4]]
|
|
| 65.350000
|-
| [[4U 2206+54]]
|
|
| 5555.000000
|-
| [[SAX J2239.3+6116]]
|
|
| 1247.000000
|-
| [[IGR J22534+6243]]
|
|
| 46.750000
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T15:57:52Z

Zainab: /* Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) =

{| class=wikitable
! Source
! Assignee
! Regions
! Pulse period
|-
| [[IGR J00370+6122]]
|
|
| 674.000000
|-
| [[2S 0114+650]]
|
|
| 10008.000000
|-
| [[4U 0115+63]]
|
|
| 3.610000
|-
| [[RX J0146.9+6121]]
|
|
| 1407.400000
|-
| [[IGR J01583+6713]]
|
|
| 469.200000
|-
| [[Swift J0243.6+6124]]
|
|
| 9.870000
|-
| [[V0332+53]]
|
|
| 4.400000
|-
| [[4U 0352+309]]
|
|
| 837.670000
|-
| [[BSD 24-491]]
|
|
| 202.500000
|-
| [[1A 0535+262]]
| Aafia
| Y
| 103.470000
|-
| [[IGR J06074+2205]]
|
|
| 373.200000
|-
| [[PSR J0635+0533]]
|
|
| 0.030000
|-
| [[MXB 0656-072]]
|
|
| 160.700000
|-
| [[4U 0728-25]]
|
|
| 103.140000
|-
| [[SGR 0755-2933]]
|
|
| 308.000000
|-
| [[LS 992]]
|
|
| 31.910000
|-
| [[Ginga 0834-430]]
|
|
| 12.300000
|-
| [[HD 77581]]
|
|
| 283.000000
|-
| [[MAXI J0903-531]]
|
|
| 14.050000
|-
| [[GRO J1008-57]]
| Aafia
| Y
| 93.500000
|-
| [[LS 1698]]
|
|
| 862.000000
|-
| [[1A 1118-61]]
|
|
| 405.000000
|-
| [[Cen X-3]]
|
|
| 4.800000
|-
| [[IGR J11215-5952]]
|
|
| 186.800000
|-
| [[IGR J11435-6109]]
|
|
| 161.800000
|-
| [[1E 1145.1-6141]]
|
|
| 298.000000
|-
| [[4U 1145-619]]
|
|
| 292.400000
|-
| [[3U 1223-62]]
|
|
| 696.000000
|-
| [[1A 1238-59]]
|
|
| 191.000000
|-
| [[HD 110432]]
|
|
| 14200.000000
|-
| [[SRGA J124404.1-632232]]
| Aafia
| Y
| 538.700000
|-
| [[3U 1258-61]]
| Aafia
| Y
| 272.000000
|-
| [[2RXP J130159.6-635806]]
|
|
| 643.000000
|-
| [[PSR B1259-63]]
|
|
| 0.050000
|-
| [[SAX J1324.4-6200]]
|
|
| 172.840000
|-
| [[HD 119682]]
|
|
| 1500.000000
|-
| [[MAXI J1409-619]]
|
|
| 503.000000
|-
| [[2S 1417-624]]
|
|
| 17.600000
|-
| [[IGR J14488-5942]]
|
|
| 33.420000
|-
| [[4U 1538-52]]
| Aafia
| Y
| 526.420000
|-
| [[XTE J1543-568]]
|
|
| 27.120000
|-
| [[2S 1553-542]]
|
|
| 9.280000
|-
| [[Swift J1626.6-5156]]
|
|
| 15.360000
|-
| [[IGR J16320-4751]]
|
|
| 1303.000000
|-
| [[IGR J16393-4643]]
| Aafia
| Y
| 908.790000
|-
| [[IGR J16418-4532]]
| Aafia
| Y
| 1246.000000
|-
| [[IGR J16465-4507]]
|
|
| 228.000000
|-
| [[IGR J16493-4348]]
|
|
| 1093.100000
|-
| [[AX J1700.2-4220]]
|
|
| 54.200000
|-
| [[OAO 1657-415]]
|
|
| 37.030000
|-
| [[IGR J17200-3116]]
|
|
| 328.200000
|-
| [[IGR J17252-3616]]
|
|
| 413.700000
|-
| [[HD 161103]]
|
|
| 3245.000000
|-
| [[AX J1749.1-2733]]
|
|
| 132.000000
|-
| [[AX J1749.2-2725]]
|
|
| 220.380000
|-
| [[GRO J1750-27]]
|
|
| 4.450000
|-
| [[IGR J17544-2619]]
|
|
| 71.490000
|-
| [[IGR J18027-2016]]
|
|
| 139.600000
|-
| [[Swift J1816.7-1613]]
|
|
| 143.690000
|-
| [[IGR J18179-1621]]
|
|
| 11.820000
|-
| [[AX J1820.5-1434]]
|
|
| 152.300000
|-
| [[IGR J18219-1347]]
|
|
| 52.460000
|-
| [[XTE J1824-141]]
|
|
| 120.000000
|-
| [[XTE J1829-098]]
|
|
| 7.850000
|-
| [[Sct X-1]]
|
|
| 112.000000
|-
| [[Ginga 1839-04]]
|
|
| 81.100000
|-
| [[Ginga 1843+009]]
|
|
| 29.480000
|-
| [[IGR J18462-0223]]
|
|
| 997.000000
|-
| [[2S 1845-024]]
|
|
| 94.720000
|-
| [[IGR J18483-0311]]
|
|
| 21.050000
|-
| [[XTE J1855-026]]
|
|
| 361.000000
|-
| [[XTE J1858+034]]
|
|
| 221.000000
|-
| [[XTE J1859+083]]
|
|
| 9.790000
|-
| [[4U 1901+03]]
| Aafia
| Y
| 2.760000
|-
| [[XTE J1906+090]]
|
|
| 89.170000
|-
| [[4U 1907+09]]
| Aafia
| Y
| 438.000000
|-
| [[AX J1910.7+0917]]
|
|
| 36200.000000
|-
| [[4U 1909+07]]
|
|
| 603.600000
|-
| [[IGR J19140+0951]]
|
|
| 5937.000000
|-
| [[IGR J19294+1816]]
|
|
| 12.440000
|-
| [[XTE J1946+274]]
|
|
| 15.800000
|-
| [[KS 1947+300]]
|
|
| 18.700000
|-
| [[4U 1954+31]]
|
|
| 19400.000000
|-
| [[2MASS J20002185+3211232]]
|
|
| 890.000000
|-
| [[W63 X-1]]
|
|
| 36.000000
|-
| [[EXO 2030+375]]
|
|
| 41.310000
|-
| [[SRGE J204319.0+443820]]
|
|
| 741.800000
|-
| [[GRO J2058+42]]
|
|
| 195.250000
|-
| [[SAX J2103.5+4545]]
|
|
| 358.610000
|-
| [[IGR J21343+4738]]
|
|
| 322.700000
|-
| [[Cep X-4]]
|
|
| 65.350000
|-
| [[4U 2206+54]]
|
|
| 5555.000000
|-
| [[SAX J2239.3+6116]]
|
|
| 1247.000000
|-
| [[IGR J22534+6243]]
|
|
| 46.750000
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T15:42:40Z

Zainab:

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting HMXB X-ray pulsars (pulse profile extractions) =

{| class=wikitable
! Source
! Assignee
! Regions
! Pulse period
|-
| [[IGR J00370+6122]]
|
|
| 674.000000
|-
| [[2S 0114+650]]
|
|
| 10008.000000
|-
| [[4U 0115+63]]
|
|
| 3.610000
|-
| [[RX J0146.9+6121]]
|
|
| 1407.400000
|-
| [[IGR J01583+6713]]
|
|
| 469.200000
|-
| [[Swift J0243.6+6124]]
|
|
| 9.870000
|-
| [[V0332+53]]
|
|
| 4.400000
|-
| [[4U 0352+309]]
|
|
| 837.670000
|-
| [[BSD 24-491]]
|
|
| 202.500000
|-
| [[1A 0535+262]]
|
|
| 103.470000
|-
| [[IGR J06074+2205]]
|
|
| 373.200000
|-
| [[PSR J0635+0533]]
|
|
| 0.030000
|-
| [[MXB 0656-072]]
|
|
| 160.700000
|-
| [[4U 0728-25]]
|
|
| 103.140000
|-
| [[SGR 0755-2933]]
|
|
| 308.000000
|-
| [[LS 992]]
|
|
| 31.910000
|-
| [[Ginga 0834-430]]
|
|
| 12.300000
|-
| [[HD 77581]]
|
|
| 283.000000
|-
| [[MAXI J0903-531]]
|
|
| 14.050000
|-
| [[GRO J1008-57]]
|
|
| 93.500000
|-
| [[LS 1698]]
|
|
| 862.000000
|-
| [[1A 1118-61]]
|
|
| 405.000000
|-
| [[Cen X-3]]
|
|
| 4.800000
|-
| [[IGR J11215-5952]]
|
|
| 186.800000
|-
| [[IGR J11435-6109]]
|
|
| 161.800000
|-
| [[1E 1145.1-6141]]
|
|
| 298.000000
|-
| [[4U 1145-619]]
|
|
| 292.400000
|-
| [[3U 1223-62]]
|
|
| 696.000000
|-
| [[1A 1238-59]]
|
|
| 191.000000
|-
| [[HD 110432]]
|
|
| 14200.000000
|-
| [[SRGA J124404.1-632232]]
|
|
| 538.700000
|-
| [[3U 1258-61]]
|
|
| 272.000000
|-
| [[2RXP J130159.6-635806]]
|
|
| 643.000000
|-
| [[PSR B1259-63]]
|
|
| 0.050000
|-
| [[SAX J1324.4-6200]]
|
|
| 172.840000
|-
| [[HD 119682]]
|
|
| 1500.000000
|-
| [[MAXI J1409-619]]
|
|
| 503.000000
|-
| [[2S 1417-624]]
|
|
| 17.600000
|-
| [[IGR J14488-5942]]
|
|
| 33.420000
|-
| [[4U 1538-52]]
|
|
| 526.420000
|-
| [[XTE J1543-568]]
|
|
| 27.120000
|-
| [[2S 1553-542]]
|
|
| 9.280000
|-
| [[Swift J1626.6-5156]]
|
|
| 15.360000
|-
| [[IGR J16320-4751]]
|
|
| 1303.000000
|-
| [[IGR J16393-4643]]
|
|
| 908.790000
|-
| [[IGR J16418-4532]]
|
|
| 1246.000000
|-
| [[IGR J16465-4507]]
|
|
| 228.000000
|-
| [[IGR J16493-4348]]
|
|
| 1093.100000
|-
| [[AX J1700.2-4220]]
|
|
| 54.200000
|-
| [[OAO 1657-415]]
|
|
| 37.030000
|-
| [[IGR J17200-3116]]
|
|
| 328.200000
|-
| [[IGR J17252-3616]]
|
|
| 413.700000
|-
| [[HD 161103]]
|
|
| 3245.000000
|-
| [[AX J1749.1-2733]]
|
|
| 132.000000
|-
| [[AX J1749.2-2725]]
|
|
| 220.380000
|-
| [[GRO J1750-27]]
|
|
| 4.450000
|-
| [[IGR J17544-2619]]
|
|
| 71.490000
|-
| [[IGR J18027-2016]]
|
|
| 139.600000
|-
| [[Swift J1816.7-1613]]
|
|
| 143.690000
|-
| [[IGR J18179-1621]]
|
|
| 11.820000
|-
| [[AX J1820.5-1434]]
|
|
| 152.300000
|-
| [[IGR J18219-1347]]
|
|
| 52.460000
|-
| [[XTE J1824-141]]
|
|
| 120.000000
|-
| [[XTE J1829-098]]
|
|
| 7.850000
|-
| [[Sct X-1]]
|
|
| 112.000000
|-
| [[Ginga 1839-04]]
|
|
| 81.100000
|-
| [[Ginga 1843+009]]
|
|
| 29.480000
|-
| [[IGR J18462-0223]]
|
|
| 997.000000
|-
| [[2S 1845-024]]
|
|
| 94.720000
|-
| [[IGR J18483-0311]]
|
|
| 21.050000
|-
| [[XTE J1855-026]]
|
|
| 361.000000
|-
| [[XTE J1858+034]]
|
|
| 221.000000
|-
| [[XTE J1859+083]]
|
|
| 9.790000
|-
| [[4U 1901+03]]
|
|
| 2.760000
|-
| [[XTE J1906+090]]
|
|
| 89.170000
|-
| [[4U 1907+09]]
|
|
| 438.000000
|-
| [[AX J1910.7+0917]]
|
|
| 36200.000000
|-
| [[4U 1909+07]]
|
|
| 603.600000
|-
| [[IGR J19140+0951]]
|
|
| 5937.000000
|-
| [[IGR J19294+1816]]
|
|
| 12.440000
|-
| [[XTE J1946+274]]
|
|
| 15.800000
|-
| [[KS 1947+300]]
|
|
| 18.700000
|-
| [[4U 1954+31]]
|
|
| 19400.000000
|-
| [[2MASS J20002185+3211232]]
|
|
| 890.000000
|-
| [[W63 X-1]]
|
|
| 36.000000
|-
| [[EXO 2030+375]]
|
|
| 41.310000
|-
| [[SRGE J204319.0+443820]]
|
|
| 741.800000
|-
| [[GRO J2058+42]]
|
|
| 195.250000
|-
| [[SAX J2103.5+4545]]
|
|
| 358.610000
|-
| [[IGR J21343+4738]]
|
|
| 322.700000
|-
| [[Cep X-4]]
|
|
| 65.350000
|-
| [[4U 2206+54]]
|
|
| 5555.000000
|-
| [[SAX J2239.3+6116]]
|
|
| 1247.000000
|-
| [[IGR J22534+6243]]
|
|
| 46.750000
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T15:20:39Z

Zainab: /* Updated list of accreting X-ray pulsars */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

{| class=wikitable
! Source
! Assignee
! Regions
! Pulse period
|-
| [[IGR J00370+6122]]
|
|
| 674.000000
|-
| [[2S 0114+650]]
|
|
| 10008.000000
|-
| [[4U 0115+63]]
|
|
| 3.610000
|-
| [[RX J0146.9+6121]]
|
|
| 1407.400000
|-
| [[IGR J01583+6713]]
|
|
| 469.200000
|-
| [[Swift J0243.6+6124]]
|
|
| 9.870000
|-
| [[V0332+53]]
|
|
| 4.400000
|-
| [[4U 0352+309]]
|
|
| 837.670000
|-
| [[BSD 24-491]]
|
|
| 202.500000
|-
| [[1A 0535+262]]
|
|
| 103.470000
|-
| [[IGR J06074+2205]]
|
|
| 373.200000
|-
| [[PSR J0635+0533]]
|
|
| 0.030000
|-
| [[MXB 0656-072]]
|
|
| 160.700000
|-
| [[4U 0728-25]]
|
|
| 103.140000
|-
| [[SGR 0755-2933]]
|
|
| 308.000000
|-
| [[LS 992]]
|
|
| 31.910000
|-
| [[Ginga 0834-430]]
|
|
| 12.300000
|-
| [[HD 77581]]
|
|
| 283.000000
|-
| [[MAXI J0903-531]]
|
|
| 14.050000
|-
| [[GRO J1008-57]]
|
|
| 93.500000
|-
| [[LS 1698]]
|
|
| 862.000000
|-
| [[1A 1118-61]]
|
|
| 405.000000
|-
| [[Cen X-3]]
|
|
| 4.800000
|-
| [[IGR J11215-5952]]
|
|
| 186.800000
|-
| [[IGR J11435-6109]]
|
|
| 161.800000
|-
| [[1E 1145.1-6141]]
|
|
| 298.000000
|-
| [[4U 1145-619]]
|
|
| 292.400000
|-
| [[3U 1223-62]]
|
|
| 696.000000
|-
| [[1A 1238-59]]
|
|
| 191.000000
|-
| [[HD 110432]]
|
|
| 14200.000000
|-
| [[SRGA J124404.1-632232]]
|
|
| 538.700000
|-
| [[3U 1258-61]]
|
|
| 272.000000
|-
| [[2RXP J130159.6-635806]]
|
|
| 643.000000
|-
| [[PSR B1259-63]]
|
|
| 0.050000
|-
| [[SAX J1324.4-6200]]
|
|
| 172.840000
|-
| [[HD 119682]]
|
|
| 1500.000000
|-
| [[MAXI J1409-619]]
|
|
| 503.000000
|-
| [[2S 1417-624]]
|
|
| 17.600000
|-
| [[IGR J14488-5942]]
|
|
| 33.420000
|-
| [[4U 1538-52]]
|
|
| 526.420000
|-
| [[XTE J1543-568]]
|
|
| 27.120000
|-
| [[2S 1553-542]]
|
|
| 9.280000
|-
| [[Swift J1626.6-5156]]
|
|
| 15.360000
|-
| [[IGR J16320-4751]]
|
|
| 1303.000000
|-
| [[IGR J16393-4643]]
|
|
| 908.790000
|-
| [[IGR J16418-4532]]
|
|
| 1246.000000
|-
| [[IGR J16465-4507]]
|
|
| 228.000000
|-
| [[IGR J16493-4348]]
|
|
| 1093.100000
|-
| [[AX J1700.2-4220]]
|
|
| 54.200000
|-
| [[OAO 1657-415]]
|
|
| 37.030000
|-
| [[IGR J17200-3116]]
|
|
| 328.200000
|-
| [[IGR J17252-3616]]
|
|
| 413.700000
|-
| [[HD 161103]]
|
|
| 3245.000000
|-
| [[AX J1749.1-2733]]
|
|
| 132.000000
|-
| [[AX J1749.2-2725]]
|
|
| 220.380000
|-
| [[GRO J1750-27]]
|
|
| 4.450000
|-
| [[IGR J17544-2619]]
|
|
| 71.490000
|-
| [[IGR J18027-2016]]
|
|
| 139.600000
|-
| [[Swift J1816.7-1613]]
|
|
| 143.690000
|-
| [[IGR J18179-1621]]
|
|
| 11.820000
|-
| [[AX J1820.5-1434]]
|
|
| 152.300000
|-
| [[IGR J18219-1347]]
|
|
| 52.460000
|-
| [[XTE J1824-141]]
|
|
| 120.000000
|-
| [[XTE J1829-098]]
|
|
| 7.850000
|-
| [[Sct X-1]]
|
|
| 112.000000
|-
| [[Ginga 1839-04]]
|
|
| 81.100000
|-
| [[Ginga 1843+009]]
|
|
| 29.480000
|-
| [[IGR J18462-0223]]
|
|
| 997.000000
|-
| [[2S 1845-024]]
|
|
| 94.720000
|-
| [[IGR J18483-0311]]
|
|
| 21.050000
|-
| [[XTE J1855-026]]
|
|
| 361.000000
|-
| [[XTE J1858+034]]
|
|
| 221.000000
|-
| [[XTE J1859+083]]
|
|
| 9.790000
|-
| [[4U 1901+03]]
|
|
| 2.760000
|-
| [[XTE J1906+090]]
|
|
| 89.170000
|-
| [[4U 1907+09]]
|
|
| 438.000000
|-
| [[AX J1910.7+0917]]
|
|
| 36200.000000
|-
| [[4U 1909+07]]
|
|
| 603.600000
|-
| [[IGR J19140+0951]]
|
|
| 5937.000000
|-
| [[IGR J19294+1816]]
|
|
| 12.440000
|-
| [[XTE J1946+274]]
|
|
| 15.800000
|-
| [[KS 1947+300]]
|
|
| 18.700000
|-
| [[4U 1954+31]]
|
|
| 19400.000000
|-
| [[2MASS J20002185+3211232]]
|
|
| 890.000000
|-
| [[W63 X-1]]
|
|
| 36.000000
|-
| [[EXO 2030+375]]
|
|
| 41.310000
|-
| [[SRGE J204319.0+443820]]
|
|
| 741.800000
|-
| [[GRO J2058+42]]
|
|
| 195.250000
|-
| [[SAX J2103.5+4545]]
|
|
| 358.610000
|-
| [[IGR J21343+4738]]
|
|
| 322.700000
|-
| [[Cep X-4]]
|
|
| 65.350000
|-
| [[4U 2206+54]]
|
|
| 5555.000000
|-
| [[SAX J2239.3+6116]]
|
|
| 1247.000000
|-
| [[IGR J22534+6243]]
|
|
| 46.750000
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T14:59:40Z

Zainab: /* Updated list of accreting X-ray pulsars */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars =
{| class="wikitable"
! Source
! Assignee
! Regions
|-
| [[IGR J00370+6122]]
|
|
|-
| [[2S 0114+650]]
|
|
|-
| [[4U 0115+63]]
|
|
|-
| [[RX J0146.9+6121]]
|
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T14:59:07Z

Zainab: /* Updated list of accreting X-ray pulsars */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars =
{| class="wikitable"
! Source
! Assignee
! Regions
|-
| [[IGR J00370+6122]]
|
|-
| [[2S 0114+650]]
|
|-
| [[4U 0115+63]]
|
|-
| [[RX J0146.9+6121]]
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T14:58:38Z

Zainab: /* Updated list of accreting X-ray pulsars */

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars =
{| class="wikitable" ! Source ! Assignee ! Regions |-
| [[IGR J00370+6122]]
|
|-
| [[2S 0114+650]]
|
|-
| [[4U 0115+63]]
|
|-
| [[RX J0146.9+6121]]
|
|-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

List of accreting X-ray pulsars

2023-11-13T14:57:55Z

Zainab:

[[Category:Accreting X-ray Pulsars]]

= List of accreting X-ray pulsars =
{| class="wikitable sortable"
! Source
! RA
! Dec
! l
! b
! Pspin (s)
! Porbit (d)
! Type
! CRSF?
! Persistent?
! Notes
|-
| [[CXOU J005047.9-731817]] || 12.699963 || -73.305018 || 302.995436 || -43.823153 || 292 || || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka SXP 292
|-

| [[RX J0059.2-7138]] || 14.803112 || -71.645828 || 302.059336 || -45.469247 || 2.76 || 82? || [[List of Be X-ray Binaries|BeXRB]]? || [[List of cyclotron line sources|C]]? || T || aka SXP 2.76
|-

| [[RX J0101.8-7223]] || 15.467910 || -72.392796 || 301.821935 || -44.712961 || 175 || || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SMC X-1]] || 19.271456 || -73.443343 || 300.414946 || -43.559342 || 0.71 || 3.892 || SG || || P || eclipsing
|-

| [[3A 0114+650]] || 19.511228 || 65.291623 || 125.709976 || 2.563488 || 9828 || 11.6 || SG || || P || 30.7 d superorbital modulation
|-

| [[4U 0115+634]] || 19.633194 || 63.742522 || 125.923515 || 1.028265 || 3.6 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || 5 or more lines
|-

| [[SXP 265]] || 23.214439 || -74.429258 || 299.185905 || -42.396387 || 264.52 || ~146 || [[List of Be X-ray Binaries|BeXRB]] || || PT || SMC region, persistent low luminosity, one type I outburst
|-

| [[RX J0146.9+6121]] || 26.750876 || 61.356573 || 129.541104 || -0.800112 || 1412 || 330? || [[List of Be X-ray Binaries|BeXRB]] || || T || aka V* V831 Cas
|-

| [[IGR J01583+6713]] || 29.577033 || 67.223185 || 129.352236 || 5.188723 || 469? || || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || controversial claim of CRSF features
|-

| [[Swift J0243.6+6124]] || 40.918432 || 61.434378 || 135.934157 || 1.428788 || 9.86 || 27.587 || [[List of Be X-ray Binaries|BeXRB]] || || T || Galactic ULX?
|-

| [[V 0332+53]] || 53.749630 || 53.173140 || 146.052090 || -2.194026 || 4.37 || 34.25 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || multiple lines
|-

| [[X Per]] || 58.846151 || 31.045836 || 163.081353 || -17.136203 || 830 || 250.3 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || P || magnetar?
|-

| [[RX J0440.9+4431]] || 70.247207 || 44.530344 || 159.847095 || -1.270023 || 203 || 155 || [[List of Be X-ray Binaries|BeXRB]] || || P || aka LS V+44 17, persistent, but with outbursts
|-

| [[LXP 169]] || 76.981153 || -68.418135 || 279.245167 || -34.534204 || 168.8 || 24.3 || [[List of Be X-ray Binaries|BeXRB]] || || T? || NS eclipsing companion
|-

| [[Swift J053041.9-665426]] || 82.675788 || -66.907566 || 276.997292 || -32.675902 || 28.78 || || [[List of Be X-ray Binaries|BeXRB]] || || T? ||
|-

| [[LMC X-4]] || 83.206501 || -66.370332 || 276.334942 || -32.529084 || 13.5 || 1.4 || SG || || P || superorbital variation ~30 d
|-

| [[1A 0535+26]] || 84.727393 || 26.315776 || 181.445049 || -2.643537 || 103 || 111.1 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J0635.2+0533]] || 98.822528 || 5.553870 || 206.149196 || -1.044562 || 0.0338 || || [[List of Be X-ray Binaries|BeXRB]] || || T || low luminosity
|-

| [[MXB 0656-07]] || 104.572030 || -7.209774 || 220.128540 || -1.767278 || 160.4 || 101.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || || aka XTE J0658-073
|-

| [[3A 0726-260]] || 112.223241 || -26.108019 || 240.281581 || -4.050430 || 103.2 || 34.5 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[RX J0812.4-3114]] || 123.118149 || -31.247807 || 249.578200 || 1.542815 || 31.9 || 80 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[GS 0834-430]] || 128.981072 || -43.185598 || 262.020238 || -1.509977 || 12.3 || 105.8 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[Vela X-1]] || 135.528560 || -40.554654 || 263.058248 || 3.929864 || 283 || 8.96 || SG || [[List of cyclotron line sources|C]] || P || eclipsing
|-

| [[GRO J1008-57]] || 152.439620 || -58.292035 || 282.996761 || -1.822544 || 93.7 || 249.48 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]]? || T || outbursts predicted precisely
|-

| [[4U 1036-56]] || 159.397094 || -56.798840 || 285.352684 || 1.433482 || 862 || || [[List of Be X-ray Binaries|BeXRB]] || || P? || aka RX J1037.5-564/LS 1698
|-

| [[1A 1118-616]] || 170.238174 || -61.916707 || 292.498528 || -0.891807 || 407 || 24? || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[Cen X-3]] || 170.312856 || -60.623776 || 292.090328 || 0.335524 || 4.8 || 2.09 || SG || [[List of cyclotron line sources|C]] || P || disk-fed HMXB
|-

| [[1E1145.1-6141]] || 176.868942 || -61.953720 || 295.489729 || -0.009704 || 297 || 14.4 || SG || || || (V* V830 Cen) varying luminosity states
|-

| [[4U 1145-619]] || 177.000032 || -62.206910 || 295.611079 || -0.240241 || 292 || 187.5 || [[List of Be X-ray Binaries|BeXRB]] || || PT ||
|-

| [[GX 301-2]] || 186.656453 || -62.770359 || 300.098061 || -0.035212 || 686 || 41.5 || SG || [[List of cyclotron line sources|C]] || P || very massive companion, strong orbital variability
|-

| [[3A 1239-599]] || 190.508997 || -60.200951 || 301.762822 || 2.649455 || 191 || || || || ||
|-

| [[GX 304-1]] || 195.321198 || -61.601845 || 304.102702 || 1.247519 || 272 || 132.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || Strong spectral parameter variations
|-

| [[SAX J1324.4-6200]] || 201.108853 || -62.016515 || 306.792444 || 0.607646 || 171 || 22 || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[2S 1417-624]] || 215.303896 || -62.698168 || 313.021369 || -1.598347 || 17.6 || 42.12 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[SAX J1452.8-5949]] || 223.207002 || -59.820983 || 317.646019 || -0.463151 || 437 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1538-522]] || 235.597300 || -52.386011 || 327.419660 || 2.163700 || 530 || 3.7 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[2S 1553-542]] || 239.452345 || -54.416113 || 327.942599 || -0.857197 || 9.3 || 29.56 || [[List of Be X-ray Binaries|BeXRB]]? || || P || Occasional outbursts
|-

| [[IGR J16194-2810]] || 244.888926 || -28.127773 || 349.119337 || 15.541316 || || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[Swift J1626.6-5156]] || 246.652146 || -51.941848 || 332.780988 || -2.002708 || 15.4 || 132.9 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T || strong flares
|-

| [[IGR J16318-4848]] || 247.951259 || -48.816876 || 335.615970 || -0.447754 || || || SG || || P || super absorbed source
|-

| [[IGR J16320-4751]] || 248.009669 || -47.874785 || 336.330340 || 0.167654 || 1309 || 8.986 || SG || || P || aka 2FGL J1632.4-4753c
|-

| [[4U 1626-67]] || 248.069509 || -67.461207 || 321.788013 || -13.091773 || 7.67 || 0.029 || UCXB || [[List of cyclotron line sources|C]] || P || Torque reversals; only UCXB with CRSF.
|-

| [[IGR J16358-4726]] || 249.124997 || -47.623903 || 337.023067 || -0.213710 || 5880 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[IGR J16393-4643]] || 249.772382 || -46.704006 || 338.001098 || 0.075060 || 912 || 3.7 || [[List of symbiotic X-ray binaries|SyXB]] || || || aka AX J1639.0-4642
|-

| [[IGR J16465-4507]] || 251.646902 || -45.117960 || 340.053530 || 0.135029 || 228 || 30.243 || || || P || aka 2MASS J16463526-4507045
|-

| [[Her X-1]] || 254.457539 || 35.342324 || 58.148987 || 37.523034 || 1.24 || 1.7 || IM || [[List of cyclotron line sources|C]] || P ||
|-

| [[AX J1700.1-4157]] || 255.018132 || -41.968217 || 344.037996 || 0.235782 || 715 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[OAO 1657-415]] || 255.202665 || -41.654882 || 344.369539 || 0.320505 || 37.7 || 10.4 || SG || [[List of cyclotron line sources|C]]? || P || eclipsing
|-

| [[4U 1700-37]] || 255.986566 || -37.844121 || 347.754446 || 2.173492 || || 3.4 || SG || || P || No pulsations; eclipsing source
|-

| [[4U 1700+24]] || 256.643762 || 23.971820 || 45.151698 || 32.990711 || 404 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 1722-363]] || 261.296681 || -36.284621 || 351.495256 || -0.354515 || ~414 || 9.74 || HMXB || || || aka IGR J17252–3616, heavily absorbed, eclipsing
|-

| [[GX 1+4]] || 263.008955 || -24.745600 || 1.937022 || 4.794969 || 170 || 1161 || [[List of symbiotic X-ray binaries|SyXB]] || || P || Pspin evolving rapidly
|-

| [[2XMM J174016.0-290337]] || 265.067079 || -29.060569 || 359.278793 || 0.929892 || 626 || || [[List of symbiotic X-ray binaries|SyXB]] || || || a. k.a. AX_J1740.2-2903
|-

| [[GRO J1744-28]] || 266.139419 || -28.744480 || 0.042075 || 0.298489 || 0.47 || 11.8 || LMXB || || T || "Bursting Pulsar"
|-

| [[GRO J1750-27]] || 267.291434 || -26.639700 || 2.370662 || 0.518408 || 4.45 || 29.82 || [[List of Be X-ray Binaries|BeXRB]]? || || P || aka AX J1749.1-2639
|-

| [[IGR J17544-2619]] || 268.605299 || -26.331274 || 3.235980 || -0.335557 || || 4.93 || SFXT? || [[List of cyclotron line sources|C]] || T ||
|-

| [[SAX J1802.7-2017]] || 270.665728 || -20.286816 || 9.417461 || 1.044121 || 139.6 || 4.57 || SG || || P || aka IGR J18027-2016
|-

| [[1RXS J180431.1-273932]] || 271.130284 || -27.659214 || 3.202710 || -2.947774 || 494 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[SAX J1808.4-3658]] || 272.114166 || -36.979379 || 355.384418 || -8.148034 || 0.0025 || 0.837 || LMXB || || || aka V* V4580 Sgr, disk accretor(?)
|-

| [[Swift J1816.7-1613]] || 274.176846 || -16.222949 || 14.587018 || 0.092428 || 142.9 || 151? || [[List of Be X-ray Binaries|BeXRB]]? || || T || [http://www.astronomerstelegram.org/?read=6253 ATel 6253] [http://www.astronomerstelegram.org/?read=1457 ATel 1457]
|-

| [[IGR J18179-1621]] || 274.467048 || -16.359400 || 14.599162 || -0.217510 || 11.82 || || || [[List of cyclotron line sources|C]]? || T || [http://www.astronomerstelegram.org/?read=1457 ATel 3947] [http://www.astronomerstelegram.org/?read=3949 ATel 3949]
|-

| [[AX J1820.5-1434]] || 275.122921 || -14.571809 || 16.473200 || 0.070620 || 152 || || || || ||
|-

| [[3A 1822-371]] || 276.445028 || -37.105158 || 356.850238 || -11.290768 || 0.59 || 0.23 || LMXB || || ||
|-

| [[Sct X-1]] || 278.857602 || -7.614004 || 24.336027 || 0.065699 || 112 || 111 || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[GS 1843+00]] || 281.403474 || 0.863160 || 33.036370 || 1.689359 || || || || || T ||
|-

| [[2S 1845-024]] || 282.075590 || -2.419729 || 30.421052 || -0.406023 || 94.8 || 242.2 || [[List of Be X-ray Binaries|BeXRB]]? || || T || aka GS 1843-02
|-

| [[XTE J1855-026]] || 283.876680 || -2.604678 || 31.076348 || -2.092060 || 361 || 6.1 || SG || || ||
|-

| [[XTE J1858+034]] || 284.678379 || 3.439739 || 36.822153 || -0.048088 || || 221 || || || T ||
|-

| [[XTE J1859+083]] || 284.778177 || 8.246352 || 41.144826 || 2.058031 || 9.8 || || || || T || [http://www.astronomerstelegram.org/?read=7037 ATel 7037]
|-

| [[4U 1901+03]] || 285.903524 || 3.190426 || 37.159966 || -1.249760 || || || || || T ||
|-

| [[XTE J1906+090]] || 286.197769 || 9.044912 || 42.497189 || 1.174872 || 89.2 || || [[List of Be X-ray Binaries|BeXRB]]? || || ||
|-

| [[4U 1907+09]] || 287.408533 || 9.829777 || 43.743566 || 0.475292 || 441 || 8.37 || SG || [[List of cyclotron line sources|C]] || P ||
|-

| [[4U 1909+07]] || 287.700872 || 7.597657 || 41.896991 || -0.811637 || 604 || 4.4 || SG || || P ||
|-

| [[IGR J19140+0951]] || 288.517606 || 9.882865 || 44.296348 || -0.468771 || || 13.55 || HMXB || || ? ||
|-

| [[IGR J19149+1036]] || 288.728311 || 10.612245 || 45.038573 || -0.313490 || || 22.25 || SG || [[List of cyclotron line sources|C]] || P || very close to GRS1915
|-

| [[IGR J19294+1816]] || 292.482927 || 18.310607 || 53.540075 || 0.115022 || 12.5 || 116? || [[List of Be X-ray Binaries|BeXRB]]? || || T ||
|-

| [[XTE J1946+274]] || 296.413975 || 27.365400 || 63.207144 || 1.395565 || 15.8 || 169.2 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[KS 1947+300]] || 297.397839 || 30.208809 || 66.098966 || 2.083585 || 18.8 || 40.4 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[3A 1954+319]] || 298.926399 || 32.096931 || 68.391941 || 1.926894 || 1.91e4 || || [[List of symbiotic X-ray binaries|SyXB]] || || ||
|-

| [[EXO 2030+375]] || 308.063627 || 37.637433 || 77.151841 || -1.241801 || 41.8 || 46.03 || [[List of Be X-ray Binaries|BeXRB]] || || T || regular outbursts
|-

| [[GRO J2058+42]] || 314.698059 || 41.776980 || 83.569877 || -2.655492 || || || || || T ||
|-

| [[SAX J2103.5+4545]] || 315.898770 || 45.751533 || 87.130252 || -0.684802 || 359 || 12.7 || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J21343+4738]] || 323.584869 || 47.633380 || 92.171608 || -3.117683 || 320.35 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || || P? || Varying levels of activity
|-

| [[Cep X-4]] || 324.877853 || 56.986219 || 99.012209 || 3.312526 || 66.32 || 20.85 || [[List of Be X-ray Binaries|BeXRB]] || [[List of cyclotron line sources|C]] || T ||
|-

| [[4U 2206+54]] || 331.984289 || 54.518433 || 100.603243 || -1.105922 || 5560 || 19.25? || SG || || P || magnetar?
|-

| [[SAX J2239.3+6116]] || 339.836831 || 61.274053 || 107.734431 || 2.362332 || 1247 || 262? || [[List of Be X-ray Binaries|BeXRB]] || || T ||
|-

| [[IGR J22534+6243]] || 343.479672 || 62.726882 || 109.923864 || 2.861557 || 46.7 || || [[List of Be X-ray Binaries|BeXRB]]? || || P? ||
|-
|}

= Location in the Galaxy =

The figure below displays the position of accreting X-ray pulsars in the Galaxy as far as known at this moment. Click on the figure for a larger version. Labels indicate the ordinal number in the first column of the table. Uncertainties in the distances are not indicated. Empty symbols represent sources for which there is no distance info in the literature; they have been artificially set to a distance of 7.6 kpc. [http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html HEASARC source class identifiers] are also given. The spiral arms are from Vallée et al. (2008)<ref name="Vallee08" />. Figure and data provided by Arash Bodaghee, SSL, UC Berkeley.

[[File:galacticdistributionxrp.png|560px|Galactic distribution of accreting X-ray pulsars.]]

{| class="wikitable"
! #
! Source
! Class
! Dist. [kpc]
!
! #
! Source
! Class
! Dist. [kpc]
|-
| 1
| GRO_J1744-28
| 1490
| 8.5
|
| 33
| 3A_0656-072
| 1316
| 3.9
|-
| 2
| GX_1+4
| 1410
| 4.5
|
| 34
| 3A_0726-260
| 1310
| 6.1
|-
| 3
| GRO_J1750-27
| 1316
| ?
|
| 35
| RX_J0812.4-3114
| 1316
| 8.8
|-
| 4
| 1RXS_J180431.1-273932
| 1410
| ?
|
| 36
| Ginga_0834-430
| 1316
| 4
|-
| 5
| AX_J1820.5-1434
| 1316
| 8.2
|
| 37
| Vela_X-1
| 1213
| 1.4
|-
| 6
| XTE_J1855-026
| 1213
| 10
|
| 38
| LMC_X-4
| 1210
| 55
|-
| 7
| Sct_X-1
| 1116
| 7
|
| 39
| GRO_J1008-57
| 1316
| 5
|-
| 8
| Ginga_1843+009
| 1316
| 12.5
|
| 40
| 4U_1036-56
| 1316
| 5
|-
| 9
| 4U_1901+03
| 1366
| ?
|
| 41
| Cen_X-3
| 1263
| 10
|-
| 10
| 4U_1909+07
| 1210
| 7
|
| 42
| 1A_1118-615
| 1366
| 5
|-
| 11
| XTE_J1906+090
| 1316
| 10
|
| 43
| 1E_1145.1-6141
| 1210
| 8.5
|-
| 12
| H_1907+097
| 1216
| 5
|
| 44
| H_1145-619
| 1316
| 3.1
|-
| 13
| 4U_1700+24
| 1400
| 0.42
|
| 45
| GX_301-2
| 1211
| 4.1
|-
| 14
| IGR_J19294+1816
| 1316
| ?
|
| 46
| SMC_X-1
| 1213
| 60
|-
| 15
| Her_X-1
| 1413
| 6.56
|
| 47
| 3A_1239-599
| 1110
| ?
|-
| 16
| XTE_J1946+274
| 1316
| 9.5
|
| 48
| RX_J0101.8-7223
| 1310
| 60
|-
| 17
| KS_1947+300
| 1316
| 9.5
|
| 49
| GX_304-1
| 1316
| 2.4
|-
| 18
| 3A_1954+319
| 1416
| 1.7
|
| 50
| SAX_J1324.4-6200
| 1310
| 10
|-
| 19
| EXO_2030+375
| 1366
| 7.1
|
| 51
| H_1417-624
| 1316
| 6
|-
| 20
| GRO_J2058+42
| 1316
| 9.0
|
| 52
| SAX_J1452.8-5949
| 1010
| 9
|-
| 21
| SAX_J2103.5+4545
| 1366
| 6.8
|
| 53
| 4U_1626-67
| 1410
| 9.0
|-
| 22
| Cep_X-4
| 1316
| 3.8
|
| 54
| H_1538-522
| 1213
| 6.4
|-
| 23
| 3A_2206+543
| 1260
| 2.6
|
| 55
| SWIFT_J1626.6-5156
| 1366
| ?
|-
| 24
| 3A_0114+650
| 1213
| 4.5
|
| 56
| AX J1700.1-4157
| 9999
| ?
|-
| 25
| H_0115+634
| 1386
| 8
|
| 57
| OAO_1657-415
| 1213
| 7.1
|-
| 26
| IGR_J01583+6713
| 1316
| 4
|
| 58
| IGR_J16358-4726
| 1110
| 7
|-
| 27
| RX_J0146.9+6121
| 1310
| 2.3
|
| 59
| IGR_J16393-4643
| 1210
| 10.6
|-
| 28
| V_0332+53
| 1366
| 7.5
|
| 60
| IGR_J16194-2810
| 1400
| 3.7
|-
| 29
| RX_J0440.9+4431
| 1310
| 3.3
|
| 61
| SAX_J1808.4-3658
| 1416
| 3.6
|-
| 30
| X_Per
| 1310
| 0.7
|
| 62
| 3A_1822-371
| 1419
| 2.5
|-
| 31
| 1A_0535+262
| 1366
| 2
|
| 63
| AX_J1740.2-2903
| 1410
| ?
|-
| 32
| SAX_J0635.2+0533
| 1310
| 5
|
|
|
|
|
|-
|}

= Gaia Distances =
'''NOTE: The distances here are for the Gaia source that is ''closest'' to the SIMBAD position for each object. This means that for objects with poorly-determined positions or no identified optical counterpart, the distance is ''INCREDIBLY SUSPECT''.''' Until someone has time to go through source-by-source and clean this up, ''you'' need to check carefully whether the ''Gaia'' source ID listed here ''actually corresponds'' to the object you are looking at.
The parallaxes are converted to distance by Bailer-Jones et al. (see [https://ui.adsabs.harvard.edu/#abs/2018arXiv180410121B/abstract this paper] and [http://www.mpia.de/homes/calj/gdr2_distances/main.html this webpage]). Again, these should be taken with a hefty grain of salt and are dependent on the priors selected by Bailer-Jones et al.
{| class="wikitable"
! Source
! Gaia source ID
! Gaia distance
|-
| [[RX J0101.8-7223]] || 4687492917085083648 || 12.3 (+2.0, -1.7)
|-

| [[3A 0114+650]] || 524924310153249920 || 6.6 (+1.6, -1.2)
|-

| [[4U 0115+634]] || 524677469790488960 || 7.2 (+1.5, -1.1)
|-

| [[RX J0146.9+6121]] || 511220031584305536 || 2.50 (+0.22, -0.19)
|-

| [[IGR J01583+6713]] || 518990967445248256 || 7.4 (+1.1, -0.9)
|-

| [[Swift J0243.6+6124]] || 465628193526364416 || 6.9 (+1.6, -1.2)
|-

| [[V 0332+53]] || 444752973131169664 || 5.1 (+1.1, -0.8)
|-

| [[X Per]] || 168450545792009600 || 0.79 +/- 0.04
|-

| [[RX J0440.9+4431]] || 252878401557369088 || 3.2 (+0.7, -0.5)
|-

| [[1A 0535+26]] || 3441207615229815040 || 2.13 (+0.26, -0.21)
|-

| [[SAX J0635.2+0533]] || 3131755943105291136 || 1.6 (+2.2, -0.8)
|-

| [[MXB 0656-07]] || 3052677318793446016 || 5.1 (+1.4, -1.0)
|-

| [[3A 0726-260]] || 5613494119544761088 || 9.5 (+3.1, -2.2)
|-

| [[RX J0812.4-3114]] || 5548261400354128768 || 6.8 (+1.2, -1.0)
|-

| [[GS 0834-430]] || 5523448270462666880 || 5.5 (+2.5, -1.7)
|-

| [[Vela X-1]] || 5620657678322625920 || 2.42 (+0.19, -0.17)
|-

| [[4U 1036-56]] || 5352018121173519488 || 5.0 (+1.1, -0.8)
|-

| [[1A 1118-616]] || 5336957010898124160 || 2.93 (+0.26, -0.22)
|-

| [[Cen X-3]] || 5337498593446516480 || 6.4 (+1.4, -1.1)
|-

| [[1E1145.1-6141]] || 5334851450481641088 || 9.1 (+2.2, -1.6)
|-

| [[4U 1145-619]] || 5334823859608495104 || 2.23 (+0.20, -0.17)
|-

| [[GX 301-2]] || 6054569565614460800 || 3.5 (+0.6, -0.5)
|-

| [[3A 1239-599]] || 6056606788861734912 || 2.9 (+2.4, -1.3)
|-

| [[GX 304-1]] || 5863533199843070208 || 2.01 (+0.15, -0.13)
|-

| [[SAX J1324.4-6200]] || 5868517973240268544 || 3.5 (+2.6, -1.7)
|-

| [[2S 1417-624]] || 5854175187681966464 || 3.8 (+2.8, -1.8)
|-

| [[SAX J1452.8-5949]] || 5878224015202026240 || 3.0 (+2.6, -1.5)
|-

| [[4U 1538-522]] || 5886085557746480000 || 6.6 (+2.2, -1.5)
|-

| [[2S 1553-542]] || 5884711610550541440 || 3.5 (+2.6, -1.5)
|-

| [[IGR J16194-2810]] || 6039227323926220544 || 2.3 (+0.8, -0.5)
|-

| [[Swift J1626.6-5156]] || 5933976985766949376 || 9.8 (+3.2, -2.4)
|-

| [[IGR J16318-4848]] || 5940777877435137024 || 5.2 (+2.8, -1.9)
|-

| [[IGR J16320-4751]] || 5941216101526297856 || 1.3 (+0.6, -0.4)
|-

| [[4U 1626-67]] || 5809528276749789312 || 3.5 (+2.3, -1.3)
|-

| [[IGR J16393-4643]] || 5942638074996489088 || 4.0 (+2.7, -1.7)
|-

| [[IGR J16465-4507]] || 5943246345430928512 || 2.7 (+0.5, -0.4)
|-

| [[Her X-1]] || 1338822021487330304 || 5.0 (+0.8, -0.6)
|-

| [[AX J1700.1-4157]] || 5966358530819164544 || 3.4 (+2.6, -1.5)
|-

| [[OAO 1657-415]] || 5966391894137386240 || 2.2 (+0.7, -0.5)
|-

| [[4U 1700-37]] || 5976382915813535232 || 1.75 (+0.24, -0.19)
|-

| [[4U 1700+24]] || 4571810378118789760 || 0.536 +/- 0.010
|-

| [[EXO 1722-363]] || 5974546387756541696 || 4.0 (+2.3, -1.3)
|-

| [[GX 1+4]] || 4110236324513030656 || 7.6 (+4.3, -2.8)
|-

| [[2XMM J174016.0-290337]] || 4060143669944331648 || 1.4 (+1.6, -0.5)
|-

| [[GRO J1744-28]] || 4057539171718068224 || 1.3 (+1.2, -0.5)
|-

| [[IGR J17544-2619]] || 4063908810076415872 || 2.7 (+0.5, -0.4)
|-

| [[SAX J1802.7-2017]] || 4070968778552176768 || 1.5 (+2.8, -0.7)
|-

| [[SAX J1808.4-3658]] || 4037867740522970240 || 5.1 (+4.3, -2.6)
|-

| [[Swift J1816.7-1613]] || 4097679145798118528 || 1.4 (+2.5, -0.7)
|-

| [[3A 1822-371]] || 6728016172687965568 || 6.1 (+2.7, -1.6)
|-

| [[GS 1843+00]] || 4278536022438800640 || 2.3 (+2.0, -1.0)
|-

| [[XTE J1855-026]] || 4255891924062617088 || 8.1 (+2.6, -1.8)
|-

| [[XTE J1858+034]] || 4280844623194795136 || 1.55 (+0.28, -0.21)
|-

| [[XTE J1859+083]] || 4310118600596712832 || 2.7 (+2.4, -1.5)
|-

| [[4U 1901+03]] || 4268774665587135488 || 2.2 (+2.2, -1.3)
|-

| [[XTE J1906+090]] || 4310649149314811776 || 2.8 (+2.4, -1.4)
|-

| [[4U 1907+09]] || 4309225217336729088 || 4.4 (+2.1, -1.3)
|-

| [[4U 1909+07]] || 4306419980916246656 || 2.6 (+2.3, -1.4)
|-

| [[IGR J19140+0951]] || 4309253392325650176 || 2.8 (+2.4, -1.4)
|-

| [[IGR J19149+1036]] || 4309736146639732352 || 3.0 (+2.5, -1.6)
|-

| [[IGR J19294+1816]] || 4323316622779495680 || 2.9 (+2.5, -1.5)
|-

| [[XTE J1946+274]] || 2028089540103670144 || 12.6 (+3.9, -2.9)
|-

| [[KS 1947+300]] || 2031939548802102656 || 15.2 (+3.7, -2.8)
|-

| [[3A 1954+319]] || 2034031438383765760 || 3.3 (+1.0, -0.7)
|-

| [[EXO 2030+375]] || 2063791369815322752 || 3.6 (+1.4, -0.9)
|-

| [[GRO J2058+42]] || 2065653598916388352 || 8.0 (+1.2, -1.0)
|-

| [[SAX J2103.5+4545]] || 2162805896614571904 || 6.4 (+0.9, -0.7)
|-

| [[IGR J21343+4738]] || 1978365123143522176 || 7.8 (+1.4, -1.1)
|-

| [[Cep X-4]] || 2178178409188167296 || 10.2 (+2.2, -1.6)
|-

| [[4U 2206+54]] || 2005653524280214400 || 3.3 +/- 0.4
|-

| [[SAX J2239.3+6116]] || 2201091578667140352 || 8.0 (+1.4, -1.1)
|-

| [[IGR J22534+6243]] || 2207277877757956352 || 8.1 (+2.3, -1.6)
|-
|}

= Updated list of accreting X-ray pulsars =
{| class="wikitable" ! Source ! Assignee ! Regions |-
| [[IGR J00370+6122]] | |-
| [[2S 0114+650]] | |-
| [[4U 0115+63]] | |-
| [[RX J0146.9+6121]] | |-
|}

= Correlation between luminosity and CRSF energy =
In recent years more and more sources have been observed at different luminosities, allowing us to find correlation between the luminosity and the cyclotron line energy. A summary of the current state of the observations can be found on this page:
[[CRSF energy as function of luminosity]]

= Assignments =
Our collaboration has assigned one or two sources to each member to take care of, i.e., to put together the most important information and keep the page up to date in case new data are available or new papers are published. [[X-ray pulsar assignments|The list]] can only be accessed if logged in.

Plot gallery

2023-11-02T11:07:13Z

Zainab:

= Remeis X-fig plot gallery =

Please add your with <code>slxfig</code> created plots! Preferably format: clickable image of your final product, leading to the s-lang code (with or without comments). When uploading pictures, please don't forget to give them a '''unique''' name, as they are all stored in one directory.

A cool website for generating color-blind friendly patterns: https://coolors.co/121619-2d4739-09814a-bcb382-e5c687. You can set the colors just by using the hex codes in xfig or tikz.

=== Mike's Fancy Plots ===
[[File:fancy_plot.png|400px|link=Mike's fancy plots (xfig example)]] Plotting spectra in the way of Mike's fancy plots

=== Plotting Model Components ===
[[File:plot_individual_components.png|400px|link=Plotting Model Components (xfig example)]] Plotting individual model components

=== Color-coded maps with png and xfig ===
[[Color-coded_maps_with_2d_histograms,_png,_and_xfig_(xfig_example)|How to plot a color-coded map (landscape) using png and xfig]]

=== Two-dimensional histograms ===

[[File:banana-plot.png|400px|link=Two-dimensional_histograms_(xfig_example)]] banana-plot with coordinate system —''[mailto:Manfred.Hanke@sternwarte.uni-erlangen.de Manfred Hanke]''

=== Compounds and multiplots ===
[[File:multiplot_and_plot.png|300px|link=compounds and multi-panel plots (xfig example)]] Compounds and multi-panel plots —''[mailto:Manfred.Hanke@sternwarte.uni-erlangen.de Manfred Hanke]''

=== parameter-space sketches ===

[[File:Chisqr_parabola.png|300px|link=Chi-squared_parabola_(xfig_example)]] [[File:Chisqr_ellipse.png|200px|link=Chi-squared_contours_(xfig_example)]]
Simple plots to sketch the meaning of sigma-values in 1-dim or 2-dim chi-squared parameter spaces. (MB: Be aware that the n-sigma projection of 2D contours on one parameter differs from the n-sigma levels obtained for only this parameter (1D), as the delta-chi^2 (or delta statistic) depends on the number of parameters.)
Author — ''[mailto:Tobias.Beuchert@sternwarte.uni-erlangen.de Tobias Beuchert] 2013-01-07 13:41''

=== Orbit plot ===

[[File:gx301_skizze_nosuz2.png|300px|link=Orbit_plot_of_GX_301-2_(xfig_example)]] Orbit plot of GX 301-2, including the average ASM lightcurve folded on the orbit. [[:File:Gx301_skizze_nosuz2.pdf|Version in better resolution (pdf)]]. Author — ''[mailto:Felix.Fuerst@sternwarte.uni-erlangen.de Felix Fürst] 2012-05-23 17:47''

=== 4 colorful landscapes ===

[[File:Color_landsc_gx301.png|300px|link=Color_Landscapes_(xfig_example)]] Color-coded maps of count-rate distribution in the pulse-profile for different epochs. Very similar to what is shown in [[Color-coded_maps_with_2d_histograms,_png,_and_xfig_(xfig_example)|an example: plotting color-coded maps with the png and xfig modules]]. Writing out the PNG with a separate routine is not neccessary anymore I think, code is a little oldish. Author — ''[mailto:Felix.Fuerst@sternwarte.uni-erlangen.de Felix Fürst] 2012-05-23 17:55''

=== Contour plot ===

[[File:Crsfcontours_xtej1946.png|300px|link=Contour_Plot_(xfig_example)]] Contour plot of the Cyclo line energy of XTE J1946+274. — ''[mailto:Sebastian.Mueller@sternwarte.uni-erlangen.de Sebastian Mueller] 2012-05-30 15:53''

=== 2D image contours ===
[[File:map2003_0_a570_cont_e.png|300px|link=2D_Map_SAA_(xfig_example)]] Map (2D histogram) of the South Atlantic Anomaly (SAA) overplotted with iso-magnetic field lines of the Earth's magnetic field. — ''[mailto:Natalie.Hell@sternwarte.uni-erlangen.de Natalie Hell]''

=== Colorful Cyg X-1 lightcurves ===
[[File:lc_cygx1.png|500px|link=Lightcurve_Cygx1_(xfig_example)]]

Combining ''RXTE''-ASM, ''Swift''-BAT and ''MAXI'' lightcurves of Cyg X-1 in one plot. The ''RXTE'' lightcurve is color-coded for the low/hard (blue) and the high/soft (red) state. The colors for ''Swift'' are the same as for ''RXTE'' at the same time, or, when the ''RXTE'' lightcurve stops, as during times with similar count rates. ''MAXI'' has its own scale from black (low/hard) to grey (high/soft). Additionally, times of Chandra observations won by our group are indicated (AO13 was scheduled but then canceled). — ''[mailto:Natalie.Hell@sternwarte.uni-erlangen.de Natalie Hell] & [mailto:Ivica.Miskovicova@sternwarte.uni-erlangen.de Ivica Miškovičová]''

=== Chandra coverage of Cyg X-1 ===
[[File:Chandra_coverage.png|300px|link=Chandra_Coverage_(xfig_example)]]

Plot of the orbital coverage of Cyg X-1 with ''Chandra'' observations, including an example of how to calculate Roche lobes with isis. —''[mailto:Manfred.Hanke@sternwarte.uni-erlangen.de Manfred Hanke]''

=== Wind structure in Cyg X-1 ===
[[File:sketch.png|400px|link=Wind_structure_of_Cyg_X-1_(xfig_example)]]

You may not know, but you can draw basically anything with slxfig! Here is a very nice example from [http://adsabs.harvard.edu/abs/2011PhDT.........9H| Manfred's PhD thesis] (see Fig. 2.62 in there for an interpretation), describing our idea of the wind structure in the Cyg X-1 system.

The plot includes a couple of very nice tricks. Slxfig provides a function to draw photons. The example also shows how to add existing eps files to the figure, and how to add your own functions to the structure saving the xfig plot. — ''[mailto:Manfred.Hanke@sternwarte.uni-erlangen.de Manfred Hanke]''

=== Linear-Logarithmic Axis ===
[[File:lin_log_axis.png|300px|link=Lin log axis (xfig example)]] Another example of a user defined axis (partially linear and logarithmic). — ''[mailto:Moritz.Boeck@sternwarte.uni-erlangen.de Moritz Boeck]''

=== Plotting images with world coordinates ===
[[File:Cygx1_iras.png|300px|link=Satellite_Picture_Zoom_(xfig_example)]] 408 MHz and IRAS images of regions centered at the position of Cygnus X-1. The WCS module is used to show sky coordinates (galactic coordinate grid on the left, RA-DEC axis labels on the right)— ''[mailto:Moritz.Boeck@sternwarte.uni-erlangen.de Moritz Boeck]''

=== Skyplot of source positions ===
[[File:source_skyplot.png|400px|link=Skyplot_of_source_positions_(xfig_example)]] Random source positions shown in an Aitoff projection of the sky in RA and DEC. The Galactic Plane is highlighted. — ''[mailto:Moritz.Boeck@sternwarte.uni-erlangen.de Moritz Boeck]''

=== Electromagnetic Spectrum ===
[[File:elmag.png|500px|link=Eletromagnetic_spectrum_(xfig_example)]]
Electromagnetic spectrum in energy, frequency and wavelength. Satellite energy ranges marked.
Original Script by [mailto:Cornellia.Mueller@sternwarte.uni-erlangen.de Cornelia Müller]
— ''[mailto:Felicia.Krauss@sternwarte.uni-erlangen.de Felicia Krauß]''

=== Monster Lightcurve Plot ===
[[File:monster_lightcurve_vg.png|400px|link=Monsterlightcurve (xfig example)]]
Lightcurves from all all-sky monitors & time of individual pointed RXTE observations of Cyg X-1. — ''[mailto:Victoria.Grinberg@sternwarte.uni-erlangen.de Victoria Grinberg]''

=== Periodic Table ===
[[File:periodictable_nh.png|400px|link=Periodic_Table_of_the_Elements_(xfig_example)]]
Draw your own periodic table in only ~120 lines of code. Data is taken from the X-ray Data Booklet 2009. —''
[mailto:Natalie.Hell@sternwarte.uni-erlangen.de Natalie Hell]''

=== Relativistic photon trajectory ===
[[File:ptrace3.png|400px|link=Lightbending_ptrace_(xfig_example)]]
Sketch of a relativistic photon trajectory. NOTE: "lbscripts" are required to execute the script. The path is set in the Script correctly, otherwise please contact me. — ''[mailto:Sebastian.Falkner@sternwarte.uni-erlangen.de Sebastian Falkner]''

=== Atomic processes ===
[[File:dr_nh.png|300px|link=Atomic_Processes_(xfig_example)]]
Make sketches of atomic processes such as di-electronic recombination (DR). Other possibilities include radiative recombination, auto-ionization, photo-ionization, ... —''
[mailto:Natalie.Hell@sternwarte.uni-erlangen.de Natalie Hell]''

=== Simple inset ===
[[Inset plot (xfig example)| Easy example for an inset]]

=== Insets and shaded regions ===
[[File:1008batlcgiant2012.png|300px|link=Insets_and_shaded_regions_(xfig_example)]]
Plotting the BAT-lightcurve of a source and shading specific regions as well as labeling them. Furthermore, adding an inset plot showing an epoch folding result here. —''
[mailto:Matthias.Kuehnel@sternwarte.uni-erlangen.de Matthias Kühnel]''

=== Insets as zoom-ins ===
[[File:gx304batlcobs.png|300px|link=GX304batlcobs_(xfig_example)]]
Plotting the BAT-lightcurve of a source and adding zooms into the lightcurve showing the available observations. —''
[mailto:Matthias.Kuehnel@sternwarte.uni-erlangen.de Matthias Kühnel]''

=== Hertzsprung-Russell diagram ===
[[File:Hr_diagram.png|300px|link=Hertzsprung-Russell_diagram_(xfig_example)]]
A schematic Hertzsprung-Russell diagram —''
[mailto:Andreas.Irrgang@sternwarte.uni-erlangen.de Andreas Irrgang]''

=== Colored data points ===
[[File:Colored_data_points.png|300px|link=Speedometer_Colorplot_(xfig_example)]]
"Speedometer"-like colormap for data points —''
[mailto:Andreas.Irrgang@sternwarte.uni-erlangen.de Andreas Irrgang]''

=== 3D Maser Disk ===
[[File:disk_map.png|300px|link=3D_Maser_Disk_(xfig_example)]]
3D Maser disk and projections on 2D. —''
[mailto:Eugenia.Litzinger@sternwarte.uni-erlangen.de Eugenia Litzinger]''

=== Angstrom and keV axes done properly in the same plot (axis coordinate transformation) ===
[[File:zoom.png|300px|link=Angstrom_to_keV_axis_transformation_(xfig_example)]]
Simple but extremely useful axis transformation; works both ways in spite of the name —''
[mailto:grinberg@space.mit.edu|Victoria Grinberg]''

=== Plotting in 3D, simple ===
[[File:object3dsimple.png|300px|link=Object3dsimple (xfig example)]]
An simple example how to create a 3D plot using vector transformations.''
[mailto:sebastian.falkner@fau.de Sebastian Falkner]''

=== Plotting in 3D ===
[[File:object3d.png|300px|link=Object3d (xfig example)]]
An example how to create a 3D plot using vector transformations.''
[mailto:sebastian.falkner@fau.de Sebastian Falkner]''

=== Calculating and plotting orbits in 3D ===

[[File:orbit3d.png|300px|link=3D orbit plots (xfig example)]]
Calculation and plots of orbits in 3D''
[mailto:matthias.kuehnel@sternwarte.uni-erlangen.de Matthias Kuehnel]''

It also defines additional TeX commands and packages for plotting purposes, such as using no bold face.

=== VLBI coordinates in 3D ===
[[File:vlbi_coordinates.png|300px]]
Displaying VLBI coordinates in 3D''
[mailto:tobias.beuchert@sternwarte.uni-erlangen.de Tobias Beuchert]''

=== Plotting a fit model ===
[[File:sedfitsmodel.png|400px|link=Plot_fit_model_(xfig_example)]]

How to plot a fit model in xfig to extend beyond the data.''
[mailto:Felicia.Krauss@fau.de Felicia Krauss]''

=== Multipanel spectral model decomposition ===
[[File:multipanel_decomposition.png|400px|link=Model decomp (xfig example)]]

Spectral model decompositions of a whole sample using multiplot. Compact and flexible code thanks to some clean file structuring and efficiently placed loops.—''[mailto:marco.fink@fau.de Marco Fink]''

=== Chi²-distribution and CDF ===
[[File:Chisqr.png|300px|link=Chisquared_Distribution_Plot_(xfig_example)]]

The Chi²-distribution and its according cumulative distribution function for a large number of degrees of freedom. Confidence levels are indicated in the CDF. Feel free to use it in your thesis.—''[mailto:marco.fink@fau.de Marco Fink]''

=== Polar Plot ===
[[File:polarplot.png|300px|link=Polar_plot_(xfig_example)]]

In the isisscripts there is a function 'xfig_polarplot_new, with which provides an easy way to plot an individual adjustable polar plot. This plot is just one very simple example, for more information see 'isis> help xfig_polarplot_new'.—''[mailto:sebastian.falkner@fau.de Sebastian Falkner]''

=== Xfig plot image ===
[[File:plotimage1.png|300px|link=Xfig_plot_image_(xfig_example)]]
[[File:plotimage2.png|300px|link=Xfig_plot_image_(xfig_example)]]

Other than the %plot_png function of the xfig_plot structure this function
aims to plot images with a (given) ARBITRARY x/y-grid in a correct way
(NOTE that .plot_png does not care for x/y values!). This also allows to
plot images with logarithmic scales without any problems! In addition
it is easy to plot gabbed images by just giving the x and y grid as bin_lo
and bin_hi.

These plots are just two very simple examples, for more information see
'isis> help xfig_plot_image'.—''[mailto:sebastian.falkner@fau.de Sebastian Falkner]''

=== Xfig plot colormap ===
[[File:plotcmap1.png|300px|link=Xfig_plot_colormap_(xfig_example)]]
[[File:plotcmap2.png|300px|link=Xfig_plot_colormap_(xfig_example)]]

The function 'xfig_plot_colormap' creates a horizontal, vertical colormap/colorscale for a given image.
For more information see 'isis> help xfig_plot_colormap'.—''[mailto:sebastian.falkner@fau.de Sebastian Falkner]''

[[Category:SLxfig]]
[[Category:Isis / Slang]]

=== Skymap with error circles ===
[[File:Skymapcirclegr.png|700px|link=Plot_skymap_(xfig_example)]]

How to plot a circles in spherical coordinates in a Hammer-Aitoff projection. (Or: how to plot the intersection of a sphere with a plane)
[mailto:Felicia.Krauss@fau.de Felicia Krauss]''

=== Plot data over different range sections ===
[[File:plot_with_gaps_jjs.png|300px|link=Plot_data_with_gaps_(xfig_example)]]

A simple example on how to plot data over a range with gaps, inserting visible markers to indicate these gaps. ''— [mailto:jakob.stierhof@fau.de Jakob Stierhof]''

=== Plot geospatial data with shapelib ===
[[File:plot_world_jjs.png|800px|link=Plot_geospatial_data_(xfig_example)]]

[[File:plot_world_vector_jjs.png|800px|link=Plot_geospatial_data_(xfig_example)]]

An exemplary use of the slang interface to the lightweight shapelib library. The library allows to read in ESRI shape files a common format for geospatial data representation. The slang wrapper is in a very early phase and together with the not very error prone shapelib c library there is lots of errors ahead of you (okay, mostly it's my fault). For example, if you try to load a file that does not exist the wrapper does not crash nicely bad faces you with a segfault. You have been warned! ''— [mailto:jakob.stierhof@fau.de Jakob Stierhof]''

=== Coloredcoded scatter plot ===
[[File:my_very_cool_colorcode.png|500px|link=Colorcoded_scatter_plot]]
Colorcoded scatter plot ''— [mailto:philipp.ph.weber@fau.de Philipp Weber] or [mailto:steven.haemmerich@fau.de Steven Hämmerich]''

=== Plot marginal and joint probabilities ===

[[File:Distribution_matrix.png|500px|link=Plot_marginal_and_joing_probabilities]]

Visualize the distribution of something in a nice triangle using one function (from the isisscripts)! ''- [mailto:jakob.stierhof@fau.de Jakob Stierhof]

= Remeis tikz plot gallery =

Information for newbies

2023-09-21T12:13:45Z

Zainab: Created page with "Welcome newbies sheet: https://www.sternwarte.uni-erlangen.de/gitlab/remeis/welcome_newbies/-/tree/e88427ed12ba49380450f4a2a4c12439cd7dfdee Category:Current Members"

Welcome newbies sheet: https://www.sternwarte.uni-erlangen.de/gitlab/remeis/welcome_newbies/-/tree/e88427ed12ba49380450f4a2a4c12439cd7dfdee

[[Category:Current Members]]

Plot gallery

2023-09-08T10:23:31Z

Zainab: