Paper Citation Record · LEDGER

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes

As of 13 August 2026, this Paper Citation Record lists 49 of 49 outbound references and 1 inbound Pith citation observation for arXiv:2501.12190.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2501.12190 v2

Coverage vector

measured 49 of 49 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:30:14.625560Z

measured 50 of 50 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T09:19:35.429829Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

49 of 49 outbound references displayed

verified exact1
verified fuzzy0
unresolved48
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 1fc888bf-fc60-472f-9f61-0f34b5031703 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.337607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2109ca5f-e0ab-440e-9454-4e1fb4f69cc5 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.343395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c95d3ddf-d1db-4201-aebe-695f099b4c4c · outbound

This paper cites D., Song Y., Takatsuka T., 2018, @doi [Reports on Progress in Physics] 10.1088/1361-6633/aaae14 , https://ui.adsabs.harvard.edu/abs/2018RPPh...81e6902B 81, 056902.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes D., Song Y., Takatsuka T., 2018, @doi [Reports on Progress in Physics] 10.1088/1361-6633/aaae14 , https://ui.adsabs.harvard.edu/abs/2018RPPh...81e6902B 81, 056902

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.348296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c45eff3-383a-4b49-ab0d-f510a93e9e4b · outbound

This paper cites V., et al., 2019, @doi [ ] 10.3847/2041-8213/ab53e7 , https://ui.adsabs.harvard.edu/abs/2019Astrophysical Journal...887L..23B 887, L23.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes V., et al., 2019, @doi [ ] 10.3847/2041-8213/ab53e7 , https://ui.adsabs.harvard.edu/abs/2019Astrophysical Journal...887L..23B 887, L23

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.354250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96a9c10d-2a89-4f9e-a32b-bd8a57a3e967 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.359729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00209d8c-2ffc-43f0-8184-e6704b4e6180 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.370865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4a6cbf5-fd08-4cf1-85e1-3153a25802ed · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.378165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4cd22b5-3870-4c89-ab75-e66e1aaca390 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.383824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 420caf6d-4a42-470c-9f47-6b1986dbd504 · outbound

This paper cites Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.389864Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 534be4c9-606e-4c1a-96f4-c689e73afce0 · outbound

This paper cites 465, Astrophysics and Space Science Library.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes 465, Astrophysics and Space Science Library

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.396172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1bd4e02c-26a4-4efd-9ed9-c4a38a2a8dcf · outbound

This paper cites Parameter constraints for accreting millisecond pulsars with synthetic NICER data.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Parameter constraints for accreting millisecond pulsars with synthetic NICER data

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.402543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a8e736e-67e5-4cc6-b8cb-8fb8f4fd4410 · outbound

This paper cites P., 2008, @doi [ ] 10.1111/j.1365-2966.2007.12353.x , https://ui.adsabs.harvard.edu/abs/2008MNRAS.384..449F 384, 449.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes P., 2008, @doi [ ] 10.1111/j.1365-2966.2007.12353.x , https://ui.adsabs.harvard.edu/abs/2008MNRAS.384..449F 384, 449

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.409825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b3461b7-959f-45c7-bcb8-a18086d6378d · outbound

This paper cites Importance Nested Sampling and the MultiNest Algorithm.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Importance Nested Sampling and the MultiNest Algorithm

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.420931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af49d847-a1c9-4b77-8ce0-8cd7d0bd579b · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.427266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c238e350-ed03-445d-932b-dc6eef4bfa54 · outbound

This paper cites The Multipolar Magnetic Field of Millisecond Pulsar PSR J0030+0451.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes The Multipolar Magnetic Field of Millisecond Pulsar PSR J0030+0451

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.432966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa100cea-7f40-4076-86ad-92da76653f36 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.439116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74e16b5c-cedc-4a35-85c4-9dce3633e893 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.444860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 153e7334-9b7c-49c2-9b9f-036511a58466 · outbound

This paper cites M., 2012, @doi [Annual Review of Nuclear and Particle Science] 10.1146/annurev-nucl-102711-095018 , http://adsabs.harvard.edu/abs/2012ARNPS..62..485L 62, 485.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes M., 2012, @doi [Annual Review of Nuclear and Particle Science] 10.1146/annurev-nucl-102711-095018 , http://adsabs.harvard.edu/abs/2012ARNPS..62..485L 62, 485

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.451444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1cd3553-a1c4-4043-add4-8c28b4ec9841 · outbound

This paper cites a ttil \.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes a ttil \

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.457289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2c0e37a5-6719-46b3-a089-66ec75bc53e2 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.463019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 692de5d5-ffd4-4c17-9cff-63124dd9c3b8 · outbound

This paper cites C., Lamb F.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes C., Lamb F

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.469382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 569706dd-5312-458c-bccf-bcc013fc723a · outbound

This paper cites V., et al., 2024, @doi [ ] 10.1051/0004-6361/202450581 , https://ui.adsabs.harvard.edu/abs/2024A&A...690A.353M 690, A353.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes V., et al., 2024, @doi [ ] 10.1051/0004-6361/202450581 , https://ui.adsabs.harvard.edu/abs/2024A&A...690A.353M 690, A353

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.475043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01b1cc4b-7c01-4056-83d2-3f1c13c147f8 · outbound

This paper cites M., Leahy D.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes M., Leahy D

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.481192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5cb8b458-8a9f-41b9-a602-9bfe3804e8ef · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.486918Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3c19cbb-33a1-4d84-b22c-9fa7d5cf38fc · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.492782Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 205f3302-2566-4900-90b1-e3bea0b84185 · outbound

This paper cites Accreting Millisecond X-Ray Pulsars.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Accreting Millisecond X-Ray Pulsars

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.498299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 488ef41b-c504-420c-9c86-888dcdd11964 · outbound

This paper cites R., Ftaclas C., Cohen J.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes R., Ftaclas C., Cohen J

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.506042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66f4ff9d-a73c-4cd9-99fd-3cc0a3f77481 · outbound

This paper cites Cambridge University Press, Cambridge, pp 168--175, @doi 10.1017/CBO9780511750809.026.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Cambridge University Press, Cambridge, pp 168--175, @doi 10.1017/CBO9780511750809.026

Reference 29

Resolution: verified exact; doi, observed 2026-08-10T17:30:14.833536Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 4c1a9cbc-e9ff-4fb1-ad4a-511b1c8661c0 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.517994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dea8857-6302-453d-bfe6-159c65e287f0 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.523966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6268360c-1a04-41d9-9e8a-b1231dcab905 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.530259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 30300545-bbf7-4089-bb8d-809ae3d98f7e · outbound

This paper cites E., et al., 2019, @doi [ ] 10.3847/2041-8213/ab481c , https://ui.adsabs.harvard.edu/abs/2019ApJ...887L..21R 887, L21.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes E., et al., 2019, @doi [ ] 10.3847/2041-8213/ab481c , https://ui.adsabs.harvard.edu/abs/2019ApJ...887L..21R 887, L21

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.536113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0571b09-3c7c-4b5e-802e-86cc581fab3d · outbound

This paper cites E., et al., 2021, @doi [ ] 10.3847/2041-8213/ac0a81 , https://ui.adsabs.harvard.edu/abs/2021ApJ...918L..27R 918, L27.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes E., et al., 2021, @doi [ ] 10.3847/2041-8213/ac0a81 , https://ui.adsabs.harvard.edu/abs/2021ApJ...918L..27R 918, L27

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.541230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9f5b7cb-05b8-4170-b5b1-b59d06a29baa · outbound

This paper cites E., et al., 2023, @doi [ Journal of Open Source Software ] 10.21105/joss.04977 , 8, 4977.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes E., et al., 2023, @doi [ Journal of Open Source Software ] 10.21105/joss.04977 , 8, 4977

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.547371Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4d13179-66bc-4d9a-9c65-a74c43165e6f · outbound

This paper cites M., Ustyugova G.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes M., Ustyugova G

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.553136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 849dd1a6-c605-415e-95ba-56cb089e1a6c · outbound

This paper cites a ttil \.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes a ttil \

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.558497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 44897c42-423b-4401-a680-62f07c27c7b2 · outbound

This paper cites S., Poutanen J., 2021, @doi [ ] 10.1051/0004-6361/202039470 , https://ui.adsabs.harvard.edu/abs/2021A&A...646A..23S 646, A23.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes S., Poutanen J., 2021, @doi [ ] 10.1051/0004-6361/202039470 , https://ui.adsabs.harvard.edu/abs/2021A&A...646A..23S 646, A23

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.563461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4020245f-b001-4ea7-9b79-f46f17117a59 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.568936Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec4588a5-dab9-480e-833c-4bfe1eed39eb · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.574549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee621b0b-9bfa-4681-bc2f-5b270f87de41 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.580124Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 91e5769b-35fa-4084-97a2-4acee230cba0 · outbound

This paper cites A., Titarchuk L.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes A., Titarchuk L

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.585402Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88c6add0-69f6-4aa9-8076-52967feefcaf · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.590056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25dc6d02-e5a8-466d-87a6-54956ccc534f · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.595382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cdeed1f-10a7-4dd2-828f-7953706f13b0 · outbound

This paper cites L., et al., 2019, @doi [Science China Physics, Mechanics, and Astronomy] 10.1007/s11433-017-9188-4 , http://adsabs.harvard.edu/abs/2019SCPMA..6229503W 62, 29503.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes L., et al., 2019, @doi [Science China Physics, Mechanics, and Astronomy] 10.1007/s11433-017-9188-4 , http://adsabs.harvard.edu/abs/2019SCPMA..6229503W 62, 29503

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.600533Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04d8b98b-1507-4964-b0e4-266f54aac6ad · outbound

This paper cites On understanding the figures of merit for detection and measurement of x-ray polarization.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes On understanding the figures of merit for detection and measurement of x-ray polarization

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.605363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cf4cfd2-8514-450d-a04f-0d5a253a5ef9 · outbound

This paper cites C., et al., 2022, @doi [JATIS] 10.1117/1.JATIS.8.2.026002 , https://ui.adsabs.harvard.edu/abs/2021arXiv211201269W 8, 026002.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes C., et al., 2022, @doi [JATIS] 10.1117/1.JATIS.8.2.026002 , https://ui.adsabs.harvard.edu/abs/2021arXiv211201269W 8, 026002

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.610511Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3731151-e9d6-4b40-9c83-b069d4ddff18 · outbound

This paper cites an unresolved cited work.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes Unresolved cited work

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.615526Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec757bc7-d443-4574-88cf-0d0381f0f34f · outbound

This paper cites N., et al., 2016, in Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes N., et al., 2016, in Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.620464Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3fffa2e6-dfe7-48a3-af1d-4a6087722897 · outbound

This paper cites write newline.

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes write newline

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T17:30:14.625560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 48bfa8e2-4780-4517-a7fc-d53fe4043de5 · inbound

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO cites this paper.

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes

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