Paper Citation Record · LEDGER

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years

As of 7 August 2026, this Paper Citation Record lists 61 of 61 outbound references and 1 inbound Pith citation observation for arXiv:2508.18195.

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

pith.paper-citation-record.v1
2508.18195 v1

Coverage vector

measured 61 of 61 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:38:04.032246Z

measured 62 of 62 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T05:10:13.912506Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

61 of 61 outbound references displayed

verified exact12
verified fuzzy1
unresolved48
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 735ec100-4a0c-4d7a-99c5-5ffed1066d38 · outbound

This paper cites A., Ackermann, M., Ajello, M., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., Ackermann, M., Ajello, M., et al

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:58.693534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db6d6210-8658-4f2e-af61-fcac15b6e1af · outbound

This paper cites A., Ackermann, M., Ajello, M., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., Ackermann, M., Ajello, M., et al

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:58.746128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9307272-658d-426e-84df-4f4362c1f55e · outbound

This paper cites 2020, ApJS, 247, 33, doi: 10.3847/1538-4365/ab6bcb.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2020, ApJS, 247, 33, doi: 10.3847/1538-4365/ab6bcb

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:58.855296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93c2573d-455b-435f-a93c-6db2d9b3d466 · outbound

This paper cites 2012, Science, 335, 189, doi: 10.1126/science.1213974.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2012, Science, 335, 189, doi: 10.1126/science.1213974

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:58.946164Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efd9abd8-0086-4de8-9f06-43db16e2c249 · outbound

This paper cites B., Baldini, L., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years B., Baldini, L., et al

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.044966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77ca7c9d-e150-4fda-8bdc-884397ec0075 · outbound

This paper cites 2013, ApJL, 777, L2, doi: 10.1088/2041-8205/777/1/L2.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2013, ApJL, 777, L2, doi: 10.1088/2041-8205/777/1/L2

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.143894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6e5d46b-a84f-4ab8-b1bb-0ff8c5fdb587 · outbound

This paper cites Pass 8: Toward the Full Realization of the Fermi-LAT Scientific Potential.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Pass 8: Toward the Full Realization of the Fermi-LAT Scientific Potential

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.231289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e63582fc-adfd-49a2-90e0-b41e710ea30d · outbound

This paper cites B., Abdo, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years B., Abdo, A

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.285872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0eb15dbc-6a37-4ed5-9329-6e085bfd0dec · outbound

This paper cites Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4).

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.401738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f57dcb73-00fb-4461-a71f-972b34952a05 · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 10

Resolution: verified exact; doi, observed 2026-08-05T16:38:06.375868Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation eee3b447-13be-40b5-8aa6-234b142f2fcf · outbound

This paper cites 2008, ApJ, 685, 384, doi: 10.1086/590399.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2008, ApJ, 685, 384, doi: 10.1086/590399

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.593553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 663af359-c787-469f-94c5-88cf6ec6556c · outbound

This paper cites K., & Kazanas, D.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years K., & Kazanas, D

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.690106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c3dc3ee3-4d7b-4c76-a519-c8a4d8e45d37 · outbound

This paper cites R., Karastergiou, A., Johnston, S., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years R., Karastergiou, A., Johnston, S., et al

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.777550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3fe8a461-da16-4ef2-a47b-482fdde1535c · outbound

This paper cites Fermi-LAT improved Pass~8 event selection.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Fermi-LAT improved Pass~8 event selection

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.870178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f83cd20-c471-4f85-a5b1-f87e5a6182a7 · outbound

This paper cites D., Blandford, R.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years D., Blandford, R

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T16:37:59.954964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b9aab72-3f73-418f-a54b-9807be51e86d · outbound

This paper cites 2012, The Astrophysical Journal, 746, 63, doi: 10.1088/0004-637X/746/1/63.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2012, The Astrophysical Journal, 746, 63, doi: 10.1088/0004-637X/746/1/63

Reference 16

Resolution: verified exact; doi, observed 2026-08-05T16:38:06.183911Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 84b92f2a-75e1-4a26-8dbe-258c23121df2 · outbound

This paper cites 2015, MNRAS, 448, 606, doi: 10.1093/mnras/stv042.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2015, MNRAS, 448, 606, doi: 10.1093/mnras/stv042

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.129279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edf5f624-f5e6-4385-91a8-caaeab7dd725 · outbound

This paper cites Y., & Beloborodov, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Y., & Beloborodov, A

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.236572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c874be05-84c0-462a-8ddf-c717829ef2bb · outbound

This paper cites Y., Cruz, F., & Spitkovsky, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Y., Cruz, F., & Spitkovsky, A

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.335120Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7247f949-c72c-4702-9ef6-3454bb39479d · outbound

This paper cites J., Kerr, M., Barr, E.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years J., Kerr, M., Barr, E

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.412703Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19980a68-8768-4175-9f70-f5e2c758ad70 · outbound

This paper cites 1999, ApJ, 511, 351, doi: 10.1086/306652.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 1999, ApJ, 511, 351, doi: 10.1086/306652

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.506858Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 013183c9-2f30-433b-8e4c-194472dc494e · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.615940Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation add50227-a642-4cc0-94af-1a8c21fd07d4 · outbound

This paper cites K., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years K., et al

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.708738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 511da993-ced4-4d38-90de-5cb2278834c3 · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.788953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88f271bc-b05c-4a09-a277-0a3e038d25b2 · outbound

This paper cites E., Lupsasca, A., & Philippov, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years E., Lupsasca, A., & Philippov, A

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.869283Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8bc29533-3dff-453d-a8d1-b9097b863ef5 · outbound

This paper cites 2023, The Astrophysical Journal, 943, 105, doi: 10.3847/1538-4357/acab05.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2023, The Astrophysical Journal, 943, 105, doi: 10.3847/1538-4357/acab05

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:00.946216Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 605127bf-76a3-4fef-a760-dd3b1a9bc161 · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.040330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abae45e2-07bf-4d85-823b-e8e3acea9cf2 · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 28

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.831646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation d76385e1-f69a-40fe-8bf6-119d5f80197c · outbound

This paper cites J., Ray, P.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years J., Ray, P

Reference 29

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.580566Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 48f812be-7bb9-4a34-bdbe-33c392cee99f · outbound

This paper cites 2011, ApJ, 732, 38, doi: 10.1088/0004-637X/732/1/38.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2011, ApJ, 732, 38, doi: 10.1088/0004-637X/732/1/38

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.267927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cdff53c7-afac-489f-bab0-970598dfbffa · outbound

This paper cites 2019, ApJ, 885, 92, doi: 10.3847/1538-4357/ab459f.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2019, ApJ, 885, 92, doi: 10.3847/1538-4357/ab459f

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.345131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d500f3e-9d39-496d-8680-840993244fbc · outbound

This paper cites 2022, ApJ, 934, 30, doi: 10.3847/1538-4357/ac7877.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2022, ApJ, 934, 30, doi: 10.3847/1538-4357/ac7877

Reference 32

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.351618Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 76f57a37-a7e0-425d-bc39-ada925bea10d · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 33

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.284776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 605215ae-b569-45f1-a33d-7503c40eb45d · outbound

This paper cites M., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years M., et al

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.622917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 214c4bfe-a978-4143-9a1f-11691fd8ee4d · outbound

This paper cites J., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years J., et al

Reference 35

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.189039Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 79a1de4e-bd3d-40ba-90b2-6405f4224c0c · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.792359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77317b2f-ff51-4fb3-9d7f-4b82b9d0309a · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.861480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3a6d1b19-2dec-48c8-a558-9f18044d6712 · outbound

This paper cites E., Johnston, S., Karastergiou, A., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years E., Johnston, S., Karastergiou, A., et al

Reference 38

Resolution: verified exact; doi, observed 2026-08-05T16:38:05.023750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 8c632c89-2733-4b93-9c5a-2e650b4954a9 · outbound

This paper cites The ubiquity of variable radio emission and spin-down rates in pulsars.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years The ubiquity of variable radio emission and spin-down rates in pulsars

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:01.982666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85e9f1ee-f5f2-45da-8935-8e89a6098a3b · outbound

This paper cites 2010, Science, 329, 408, doi: 10.1126/science.1186683.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2010, Science, 329, 408, doi: 10.1126/science.1186683

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.090207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9993d77-48f8-4f6b-a3b4-a510d1842d52 · outbound

This paper cites G., Stappers, B.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years G., Stappers, B

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.204595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ddef781-5351-4278-a1d5-602c7ce0dd7f · outbound

This paper cites 2014, Monthly Notices of the Royal Astronomical Society, 437, 21, doi: 10.1093/mnras/stt1828.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2014, Monthly Notices of the Royal Astronomical Society, 437, 21, doi: 10.1093/mnras/stt1828

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.303568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b50852d6-d6a8-4c5d-a63c-f723794d423a · outbound

This paper cites 2022, Annual Review of Astronomy and Astrophysics, 60, 495, doi: 10.1146/annurev-astro-052920-112338.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2022, Annual Review of Astronomy and Astrophysics, 60, 495, doi: 10.1146/annurev-astro-052920-112338

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.408357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e72e29d7-5c85-4164-ae1f-02191d14bc3b · outbound

This paper cites 2020, Physical Review Letters, 124, 245101, doi: 10.1103/PhysRevLett.124.245101.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2020, Physical Review Letters, 124, 245101, doi: 10.1103/PhysRevLett.124.245101

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.514657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bfce2f3b-8b2f-4d0f-aadc-e4b3dd9dd740 · outbound

This paper cites A., & Spitkovsky, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., & Spitkovsky, A

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.615395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e698d4a4-9e42-46f7-9b9a-231b0e1127c7 · outbound

This paper cites A., & Spitkovsky, A.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., & Spitkovsky, A

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.715522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8f542ea-0187-44d0-9089-cc2cf6c71aeb · outbound

This paper cites A., Spitkovsky, A., & Cerutti, B.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., Spitkovsky, A., & Cerutti, B

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:02.784744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a820bc9-d360-4317-b67b-254b0a51075c · outbound

This paper cites M., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years M., et al

Reference 48

Resolution: verified exact; doi, observed 2026-08-05T16:38:04.782906Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 96f385a4-41fa-4f4f-9f4d-1ceb4bc94e2f · outbound

This paper cites S., Bhattacharyya, B., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years S., Bhattacharyya, B., et al

Reference 49

Resolution: verified exact; doi, observed 2026-08-05T16:38:04.634368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation e8d4c65e-8dc6-4e83-966b-5a9f810044db · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.046830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f944c4ff-5658-4f0d-af00-81e6e4e1613e · outbound

This paper cites D., Norris, J.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years D., Norris, J

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.103327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e4d6f13-bfdb-47b1-9755-cb2eb58bb709 · outbound

This paper cites W., Weltevrede, P., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years W., Weltevrede, P., et al

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.192040Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e94c43ac-5635-4d42-b99a-41c97c214c95 · outbound

This paper cites A., Abdollahi, S., Ajello, M., et al.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., Abdollahi, S., Ajello, M., et al

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T16:38:06.894985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 8087e423-7a12-492e-bcf8-5257c93991d2 · outbound

This paper cites Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-08-05T16:38:04.448047Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 7439c055-09c3-4d07-bb26-91844969916c · outbound

This paper cites 2006, ApJL, 648, L51, doi: 10.1086/507518.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years 2006, ApJL, 648, L51, doi: 10.1086/507518

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.481308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e839d57-4058-4029-8227-7e6e81698171 · outbound

This paper cites Simulations of pulsar wind formation.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Simulations of pulsar wind formation

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.591606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84ea57c3-c9f0-4fcc-9a22-9ce720cb2e38 · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.692037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07cec614-2f75-4e8b-a78e-472d954a29af · outbound

This paper cites an unresolved cited work.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.753905Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3df790ef-785c-43e6-b30c-9844a2639ebc · outbound

This paper cites N., & Arons, J.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years N., & Arons, J

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.852902Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 864b7f69-a752-42cb-9832-ab2bea9e84ac · outbound

This paper cites N., & Johnston, S.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years N., & Johnston, S

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-05T16:38:03.971874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4b8dad5-8529-48d3-937d-ee069efea56f · outbound

This paper cites A., Cherry, M.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years A., Cherry, M

Reference 61

Resolution: verified exact; doi, observed 2026-08-05T16:38:04.224411Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Pith citing papers

Observation 86a810bd-d878-4eae-845a-b7910da68036 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years

Reference 104

Resolution: unresolved; no resolver link, observed 2026-07-12T05:10:13.912506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.