{"as_of":"2026-08-13T12:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bae82285ce93e11899a1506dd1e4f732e10468f0d6d27057f23dbc7635778655","coverage":[{"denominator":83,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":83,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T18:51:27.071611Z","state":"measured"},{"denominator":83,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":83,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2501.10999/citation-record","integrity":"/paper/2501.10999/integrity","json":"/paper/2501.10999/citation-record.json","paper":"/paper/2501.10999"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.765591Z","title":"2017, Nature Astronomy, 1, 854, doi: 10.1038/s41550-017-0266-2","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.765591Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d15d17abb4857b7429ee3724da68091a9cf3421f56b126226c0c8c1ecaed069b","observation_id":"638a88a7-eb22-45f6-ba7c-81728e02c103","resolution":{"observed_at":"2026-08-10T18:51:26.765591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.769762Z","title":"M., Kaspi, V","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.769762Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:3f2d27f3677c70973397fe63379ad007776ad1c022f29747ad933c4a74e4b206","observation_id":"a37faf29-3a71-4048-b0d7-fc0b7f88f863","resolution":{"observed_at":"2026-08-10T18:51:26.769762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/739/1/39","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.848382Z","title":"V., Ransom, S","venue":null,"work_id":"f239696f-9668-4999-aa7e-55fdc78fcfce","year":2011},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.773785Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:08576f1f87955ba21282d35b353cbfe5525a25c6a7a937811bec5b986c32936e","observation_id":"33df566f-71a3-4bb8-b7bf-88f52af32c31","resolution":{"observed_at":"2026-08-10T18:51:27.853107Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.777805Z","title":"1934, Proceedings of the National Academy of Science, 20, 259, doi: 10.1073/pnas.20.5.259","venue":null,"work_id":null,"year":1934},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.777805Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d21cdd509a950498b1e90e8b4199af060fe27f433712c774cb69a142526f0717","observation_id":"f16e4296-7eaa-429e-abbd-0d108bfa00a4","resolution":{"observed_at":"2026-08-10T18:51:26.777805Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9708169","last_updated":"1997-08-19T13:37:36Z","snapshot_observed_at":"2026-07-07T01:18:06.972957Z","submitted_at":"1997-08-19T13:37:36Z","title":"The X-ray luminosity of rotation-powered neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9708169","snapshot_observed_at":"2026-08-10T18:51:26.782501Z","title":"1997, A&A, 326, 682, doi: 10.48550/arXiv.astro-ph/9708169","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.782501Z"},"links":{"cited_paper":"/paper/astro-ph/9708169","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:70c1ad4a3972a2e12bb8f43ed6d5ba7b9ace5ae12ec6856747df99e6c4ec13c8","observation_id":"e230dc23-8d58-477e-85fe-33732e7f7401","resolution":{"observed_at":"2026-08-10T18:51:26.782501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9806381","last_updated":"1998-06-30T12:56:18Z","snapshot_observed_at":"2026-08-04T02:45:36.706478Z","submitted_at":"1998-06-30T12:56:18Z","title":"The X-ray emission properties of millisecond pulsars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9806381","snapshot_observed_at":"2026-08-10T18:51:26.786703Z","title":"1999, A&A, 341, 803, doi: 10.48550/arXiv.astro-ph/9806381","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.786703Z"},"links":{"cited_paper":"/paper/astro-ph/9806381","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:69081f25f391f329f05c9cd708edc291ff13e337f8fcf39601a5acd21df7aca9","observation_id":"e6aa38d0-9a3e-48ae-a4c9-71ef6927f17b","resolution":{"observed_at":"2026-08-10T18:51:26.786703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/424498","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.811908Z","title":"C., Tennant, A","venue":null,"work_id":"ffaccd6c-9681-43fb-af25-adcae00d1b85","year":2004},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.791083Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:7b1055d57f9fdf68eb29dcb7160c390daeb61c090437aeb98bc8a8a5eaf0e26f","observation_id":"d2480c0d-e0f9-480e-9871-d79798e168b4","resolution":{"observed_at":"2026-08-10T18:51:27.815922Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.794662Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.794662Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:7db53586b2011dec158238937b37d16ff9fd50652e2c8d9fa5491a1e8517c564","observation_id":"ea80ea4c-e96a-4dc0-be58-8bdd30a7398c","resolution":{"observed_at":"2026-08-10T18:51:26.794662Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.798458Z","title":"S., Ransom, S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.798458Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:c6ae651a4174a373ca7e7e7d0d85a0bf9d11030003ab55de8b9de77bf0f0b478","observation_id":"bf54d507-f0b9-4492-810f-f93aa5a5ab01","resolution":{"observed_at":"2026-08-10T18:51:26.798458Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stad400","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.785841Z","title":"2023, MNRAS, 520, 4068, doi: 10.1093/mnras/stad400","venue":null,"work_id":"1bc696d6-5bf1-475c-b9fe-10e7675de0c5","year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.802141Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:ca2afa9e563e8132e0c054dc8e5858d148478e59f2a17d74065f8cd0fa9ac07a","observation_id":"265d011a-9f93-459d-b7e8-c7f2a14e0a6c","resolution":{"observed_at":"2026-08-10T18:51:27.790881Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/311117","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.773675Z","title":"S., Gil, J., & Zhang, L","venue":null,"work_id":"df4f2bc8-6aa6-4acd-95da-242ebe6090c8","year":1998},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.806120Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:0b832a27e26920d5e56a808e997be1cd31f64769d8fd48c86f222a2c45b954a2","observation_id":"9a23d822-d932-4a3b-b5ea-55f8f31328ce","resolution":{"observed_at":"2026-08-10T18:51:27.777568Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.810289Z","title":"S., Ho, C., & Ruderman, M","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.810289Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:fec35ac6e2a096fdfdad88c923e990211b487cbc33aca82c606021fdf1f33837","observation_id":"e54329c7-c40c-40b5-9bc9-ab71702010b7","resolution":{"observed_at":"2026-08-10T18:51:26.810289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207156","last_updated":"2003-01-28T16:07:00Z","snapshot_observed_at":"2026-07-07T00:27:17.742565Z","submitted_at":"2002-07-08T08:32:31Z","title":"NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207156","snapshot_observed_at":"2026-08-10T18:51:26.814168Z","title":"M., & Lazio, T","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.814168Z"},"links":{"cited_paper":"/paper/astro-ph/0207156","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:b1328bcc7d5a1af02e08fd3160076d55c2cd4bd75a61b2b0a16df4b0186dde2d","observation_id":"de7249e1-b6d6-40e6-ac40-4160f278d24c","resolution":{"observed_at":"2026-08-10T18:51:26.814168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa287","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.744075Z","title":"2020, MNRAS, 493, 1874, doi: 10.1093/mnras/staa287","venue":null,"work_id":"13bfb1a5-3bf3-46fa-8db9-0f3c23852d15","year":2020},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.818118Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:a6721ef5298044ce6966c59314fdcd908372738cc3ef308778f2cf686daf51f2","observation_id":"2bf8eb1e-3d3d-4b7b-af59-4df4f5aacd22","resolution":{"observed_at":"2026-08-10T18:51:27.748516Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.821748Z","title":"2024, The Astronomer’s Telegram, 16875, 1","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.821748Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:cc9962c61d9f965e5fe380813d5eb263d47c095670ffbc9ec4e7a31419dddabb","observation_id":"bbf08345-c843-4c8c-8820-af54012eb55a","resolution":{"observed_at":"2026-08-10T18:51:26.821748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201834590","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.732243Z","title":"2019, A&A, 623, A115, doi: 10.1051/0004-6361/201834590","venue":null,"work_id":"2e1c3891-721c-48b3-8b1b-58acbaa9347d","year":2019},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.825255Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:de74abf78cc97c101892889402ce5c9f5a5c50aa362929996b56ae07ef9a470d","observation_id":"c9d09075-c231-4517-b5b9-f90163b0d466","resolution":{"observed_at":"2026-08-10T18:51:27.736478Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.828862Z","title":"N., Primini, F","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.828862Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:9df1417785359ecb7aad449eddb39e729af776ee8da841fcf095e0a6eace17cf","observation_id":"d0287b03-125e-4892-afff-d8b5b5205d5d","resolution":{"observed_at":"2026-08-10T18:51:26.828862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.832387Z","title":"N., Evans, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.832387Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:8cb986d258b5a30ea02e207e7dd735d090dc6ff363f5e688c624eb278f936d1d","observation_id":"ccc358c9-17d6-44eb-8fb3-5164d6afd758","resolution":{"observed_at":"2026-08-10T18:51:26.832387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.836251Z","title":"2014, in The X-ray Universe 2014, ed","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.836251Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:b2582420ca5ebc9d21095930fed00aa6a3c285cc3a5e830b45de2c08d0c0fc56","observation_id":"0e10d122-1ab6-4a35-be75-a66929d2d42f","resolution":{"observed_at":"2026-08-10T18:51:26.836251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.840003Z","title":"V., Halpern, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.840003Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d4c8fed989cf0eb2c042ae40bfa22a3da66bd54c454b106e548a747f22d3fc7d","observation_id":"7360c2ba-74df-4cda-9618-e94ceb48b119","resolution":{"observed_at":"2026-08-10T18:51:26.840003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.843516Z","title":"S., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.843516Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:743db09f2853503a86ebe7f5fdc9cdf7bbd71a271d6545f12ac9e157992adc2b","observation_id":"47f57fa8-dccb-42a4-b8ec-4d480e605f2d","resolution":{"observed_at":"2026-08-10T18:51:26.843516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.846935Z","title":"L., Wang, C., Wang, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.846935Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:353920c1621eb111bdd472a400b52089f1a203bf02e2df1cd6b2b6f377d11fe9","observation_id":"9fa9e22f-39c8-4702-a990-0cb7b2b016a3","resolution":{"observed_at":"2026-08-10T18:51:26.846935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.15961","last_updated":"2025-01-31T14:54:49Z","snapshot_observed_at":"2026-08-12T13:39:32.240840Z","submitted_at":"2024-11-24T19:25:41Z","title":"The FAST Galactic Plane Pulsar Snapshot survey: VI. The discovery of 473 new pulsars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.15961","snapshot_observed_at":"2026-08-10T18:51:26.850545Z","title":"L., Zhou, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.850545Z"},"links":{"cited_paper":"/paper/2411.15961","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:2b24258bcbcf75758289a91752daa7e66071e16ba5a3941020937e8e7a1c68de","observation_id":"3369f9e0-4436-4dd8-9b50-1f45ed3a05fb","resolution":{"observed_at":"2026-08-10T18:51:26.850545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.854305Z","title":"2021, ApJ, 923, 249, doi: 10.3847/1538-4357/ac30e2","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.854305Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:b95241d0ac47dc4cf9b128c5adba12532b5b7f00eb8db28eeddddcb0c34cf86c","observation_id":"cd13856c-cbf5-489d-ae37-3eafbd3e6849","resolution":{"observed_at":"2026-08-10T18:51:26.854305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.857839Z","title":"2018, MNRAS, 480, 3655, doi: 10.1093/mnras/sty2075","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.857839Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:538fc61229711fe1a78e76004b0f0eea2119729b75799c9134cc95c37faccecd","observation_id":"73649b7d-eb85-405e-ab4b-cb8164e1a83c","resolution":{"observed_at":"2026-08-10T18:51:26.857839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/422408","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.665932Z","title":null,"venue":null,"work_id":"297a9c72-7d22-44e4-87de-3909039158ea","year":2004},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.861571Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:bf250a1afe01c90c84558c2a7ef8d0aedbbdbd9a5fb5ba1c0b095bedd84aa89a","observation_id":"085b9d3b-f626-4847-96af-c0a89dcc5aff","resolution":{"observed_at":"2026-08-10T18:51:27.669844Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.865434Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.865434Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:aa354d51464afbebd8558a03f4430997debb9f7174bda6505ba91759e90379ed","observation_id":"626fc77d-b478-4e3a-a92d-687157091929","resolution":{"observed_at":"2026-08-10T18:51:26.865434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.869265Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.869265Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:3e79fd45467b5a48f31ffdf9ffc985c0f57800ddded7b0e80d609d96bfdd2dfd","observation_id":"9ec5e5d6-28ee-4e2a-809c-a0c692578cab","resolution":{"observed_at":"2026-08-10T18:51:26.869265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stab025","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.641768Z","title":"2021, MNRAS, 502, 390, doi: 10.1093/mnras/stab025","venue":null,"work_id":"b3bae11d-2642-4ef8-9f83-d459c92ee8b0","year":2021},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.873132Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:91c5af5548809070dd54a5ff125add2270921b99b836ca28ea1a36f06ffe9abc","observation_id":"9f419c17-50ce-417e-a7a9-544768d6cd32","resolution":{"observed_at":"2026-08-10T18:51:27.645417Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.876938Z","title":"2019, Science China","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.876938Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:0a38d01dfc0c6f813e05e66322aa78a5aa919989866468cfb8f3deea5f8891b0","observation_id":"9fa92ee0-9c4d-4d13-b8b0-fcf1f99ed09d","resolution":{"observed_at":"2026-08-10T18:51:26.876938Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.880493Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.880493Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:4be05aa0dbfc00ae039da7bbd6efd96e7b72e2aaadf83527203d7c88d1ddb8d0","observation_id":"b06f2d84-739f-440c-a7c0-efe31ed1771f","resolution":{"observed_at":"2026-08-10T18:51:26.880493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.884777Z","title":"N., Lyne, A","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.884777Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:06122b22e5d0adde5747590f8a9917d24532d3ac982709715f4e53a154ba3af7","observation_id":"338389f7-2559-4c30-a734-981ef3c57660","resolution":{"observed_at":"2026-08-10T18:51:26.884777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.888357Z","title":"A., Ward, C","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.888357Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:de355d354748018a7c030e532137c7fa6f6e39821b1ad8340a60622e9f24a4b4","observation_id":"be7b71d0-2913-41c0-8fdd-069be951690f","resolution":{"observed_at":"2026-08-10T18:51:26.888357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202037873","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.611488Z","title":"I., Hui, C","venue":null,"work_id":"e4b6c7f6-0a21-436a-a916-f44289a7409b","year":2020},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.891832Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:c50a4b7d12decc2dcb637576d5d544ee5cffc54d09f6e197f6f506add2a0525c","observation_id":"021d3139-d609-4fbc-95eb-5e53f71f6a89","resolution":{"observed_at":"2026-08-10T18:51:27.615194Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aad284","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.600467Z","title":"Y., Takata, J., et al","venue":null,"work_id":"860e9db5-6da6-4ffb-922b-55d593fcfb88","year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.895361Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:92a465510029c3086d5331619543f6457c25021a7126baf4851cda614e1d61f4","observation_id":"e2db43ee-232e-4e00-bc95-b5d56c0f4eed","resolution":{"observed_at":"2026-08-10T18:51:27.604233Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.899237Z","title":"2018, IEEE Microwave Magazine, 19, 112, doi: 10.1109/MMM.2018.2802178","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.899237Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:1615d45cbaca81b93795fb861c70e7a1550e4cbf2480658a57626ac355242ec2","observation_id":"7886ab45-a585-4dd6-993d-9e4bfb444c1e","resolution":{"observed_at":"2026-08-10T18:51:26.899237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.902786Z","title":"2008, ApJ, 682, 1166, doi: 10.1086/589495","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.902786Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:1bb73a9a3335d7ff0c0dcea27f4d9fc5fdea2599c499327dea7d0a2e3d449eca","observation_id":"2da394ed-410e-4659-8b40-f3c744d78d9c","resolution":{"observed_at":"2026-08-10T18:51:26.902786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/2041-8205/793/1/l8","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.583341Z","title":null,"venue":null,"work_id":"a4fcc54a-f0d7-48d8-9030-7b05dceffc10","year":2014},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.906248Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:14eca63e8e7e41c7e46fd26e3533499621bf13cf453ca8ba3db0ad6da345e5e0","observation_id":"9bb61639-e0ea-403f-8230-dea582243b1e","resolution":{"observed_at":"2026-08-10T18:51:27.586987Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.910035Z","title":"C.-C., Takata, J., Hwang, C.-Y., & Liang, J.-S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.910035Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:36196a1ccc86c9ccb64702118fff150a4dec3f329840077353d854259b3caf48","observation_id":"f8967d7c-c574-4585-b2f7-6b1b4524b065","resolution":{"observed_at":"2026-08-10T18:51:26.910035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.913696Z","title":"D., Gotthelf, E","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.913696Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d5df14cef96d847fe5ea5dfa41a0a5334807dd44e9802f73602d5c30e0bebf09","observation_id":"2bf3e473-b9c4-4b52-a3f1-cdae564d9212","resolution":{"observed_at":"2026-08-10T18:51:26.913696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.917435Z","title":"2012, Pulsar Astronomy","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.917435Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:dcc6f7bde1e14e2a03a1c51adfe5c1701266a3662106da09d90546b66d851d4a","observation_id":"353124f0-96a3-431f-a309-e21037650ba3","resolution":{"observed_at":"2026-08-10T18:51:26.917435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.921017Z","title":"N., Hobbs, G","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.921017Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:2a29a0215eb18768d5e5272953c92e813082cbd0e390d18bc09376bc26d2e412","observation_id":"ee77e85e-2c9f-4087-88aa-6af4f123784b","resolution":{"observed_at":"2026-08-10T18:51:26.921017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.1748","last_updated":"2012-05-08T17:16:00Z","snapshot_observed_at":"2026-07-06T02:47:44.643408Z","submitted_at":"2012-05-08T17:16:00Z","title":"The X-ray behaviour of Fermi/LAT pulsars","version":1},"cited_work":{"arxiv_id":"1205.1748","doi":"10.48550/arxiv.1205.1748","metadata_source":"pith","pith_arxiv_id":"1205.1748","snapshot_observed_at":"2026-08-11T00:16:15.729268Z","title":"The X-ray behaviour of Fermi/LAT pulsars","venue":"astro-ph.HE","work_id":"4a7aa020-8f87-4a01-8330-b0b9b79600c2","year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.924553Z"},"links":{"cited_paper":"/paper/1205.1748","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:30131cbc628335ae83f41c682809553f6e3bce0fc88bff89715272c828767d2c","observation_id":"ab9e7a51-7ad2-4e14-8e60-4be7f3545c55","resolution":{"observed_at":"2026-08-10T18:51:27.561599Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/0004-637x/819/1/40","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.542689Z","title":"2016, ApJ, 819, 40, doi: 10.3847/0004-637X/819/1/40","venue":null,"work_id":"b9229b31-34c1-4462-a5be-a7888f022790","year":2016},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.928651Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:2a1d9a3fb3eed623b8021735488ba55bf6a3b0f306d3726d5775ef415e7f34a0","observation_id":"7360c6d6-503d-4382-bad4-9cb515ac7c47","resolution":{"observed_at":"2026-08-10T18:51:27.546675Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/795/2/168","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.428940Z","title":"2014, ApJ, 795, 168, doi: 10.1088/0004-637X/795/2/168","venue":null,"work_id":"5d02c8b2-be02-4577-af4a-2ce17a872a42","year":2014},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.932047Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:7b368a34384cc606db7d3ef7ee424ab29f2fd811e0406a21e8bdc48aad73b7bf","observation_id":"763e7d5a-3f85-4760-b779-e36d39d807ac","resolution":{"observed_at":"2026-08-10T18:51:27.432451Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/497327","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.418439Z","title":"E., Zane, S., Cropper, M., Vestrand, W","venue":null,"work_id":"bc5f4722-cfa0-4b10-a85d-999a6911ae44","year":2006},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.935664Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:51adea66d974ad75824df573e09abf8f3aef8016e04a676ce7f3a5180fcc840a","observation_id":"736db66d-29f2-4a72-b8ec-48d1e4e6a703","resolution":{"observed_at":"2026-08-10T18:51:27.422252Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.asr.2009.12.011","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.406738Z","title":null,"venue":null,"work_id":"5a77bbc1-ea0e-4bf9-a460-32cda578520f","year":2011},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.939504Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:a0c7cecae51d246acfb2c8774104f2d194cee6435d22f2651eb8e1eb93bd1228","observation_id":"220c15af-7c43-4f3d-814d-efa4196e600e","resolution":{"observed_at":"2026-08-10T18:51:27.411171Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/776/2/104","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.396057Z","title":"J., McLaughlin, M","venue":null,"work_id":"baf41cb5-0ded-4725-a74e-c0a6bdfb723f","year":2013},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.943063Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:1aa3b34fc0c79e8a67b6ba3685a12521f427381f0b059c8da9139115077146bf","observation_id":"19a595db-abc2-4d18-b29c-2c5ab6c6859e","resolution":{"observed_at":"2026-08-10T18:51:27.399678Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.946711Z","title":"P., Baganoff, F","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.946711Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:2dc82fe64edcb91ca0d13a928f8668f966eeef4248c13b701a726a2c9c483de2","observation_id":"353e6577-7b50-49a1-b100-469e2599d9a3","resolution":{"observed_at":"2026-08-10T18:51:26.946711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.950237Z","title":"2011, International Journal of Modern Physics D, 20, 989, doi: 10.1142/S0218271811019335","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.950237Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:a71a008b9f04a83f57725ec00e344035669146f0a4e30787c71961b9a8efd2c7","observation_id":"482cb72c-e9f4-40ce-86b5-04b015da0464","resolution":{"observed_at":"2026-08-10T18:51:26.950237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.953711Z","title":"Y., Romani, R","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.953711Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:8d2cd37ada00612a83ff2413d89cea9419ce8a690cd11bde0ea031be477ecef6","observation_id":"733d4c74-49d6-4859-9945-49b30c354510","resolution":{"observed_at":"2026-08-10T18:51:26.953711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.957665Z","title":"G., Jiang, P., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.957665Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:86a859d49764587de6804221b1743f14bb2c26c49d6e6dd2690d30f37cb9943c","observation_id":"8f362b83-435c-49d0-8eaf-0babbe356152","resolution":{"observed_at":"2026-08-10T18:51:26.957665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:28.050691Z","title":"2012, in American Institute of Physics Conference Series, Vol","venue":null,"work_id":"b084352d-9e65-44cc-a98d-2fafc4305c16","year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.961438Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:4f26166adb9823dc97b2af4c8865eaf4ac16b780ab7894439dc2703b83efd4cf","observation_id":"5db41ed0-228e-45b0-a7f0-8294df886fcb","resolution":{"observed_at":"2026-08-10T18:51:28.055922Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.4772264","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.357732Z","title":"Hofmann, & F","venue":null,"work_id":"1121d0e0-208c-4894-bcdb-3905b3e801bb","year":null},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.965102Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:08362db049cdde3d9b1d07cb159e1da8453f7d4b7ebdf73826fe7a5bc6430981","observation_id":"3b9b973d-f706-4b5e-a2a2-3bf15e6b8b24","resolution":{"observed_at":"2026-08-10T18:51:27.361768Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnrasl/slv013","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.346638Z","title":"M., et al","venue":null,"work_id":"9efd7703-1174-4db4-9a8e-fef328526ab5","year":2015},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.968960Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:c992c277763f5e95cc789232c311df5b6ee182e887726ae99ed393ca4c6fb07c","observation_id":"19491e9f-b333-40fb-becd-3fe52550c5de","resolution":{"observed_at":"2026-08-10T18:51:27.350509Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.972683Z","title":"2023, ApJ, 945, 66, doi: 10.3847/1538-4357/acba0e","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.972683Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:117a716640ce2fc61421154f4a43b7fcc0be88d06aa42cfc45a7ae5de323fc6c","observation_id":"a0a7db8e-b9a0-42d4-b646-ee26d6cf9dd8","resolution":{"observed_at":"2026-08-10T18:51:26.972683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/744/2/105","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.327393Z","title":"J., Guillemot, L., Allen, B., et al","venue":null,"work_id":"42e44543-278e-4f30-9ace-c526de2f5706","year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.976440Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:552d8f4e48960fb7119d2bbc239e35682a4ea8b69ac3d88d5c9baf51f8102f4e","observation_id":"f9fe7129-9306-48ab-a4dc-db36346c6f83","resolution":{"observed_at":"2026-08-10T18:51:27.331130Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.980187Z","title":"2002, A&A, 387, 993, doi: 10.1051/0004-6361:20020472","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.980187Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:cdf47f73aba7e82c1b9f319fdfae796f0b420100f570f430322b4d0eb48a77bd","observation_id":"8b59d394-42c3-45b6-94e0-41c5c20c4204","resolution":{"observed_at":"2026-08-10T18:51:26.980187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.983887Z","title":"A., Houck, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.983887Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:fe4c35b3aa0b2c99fc534027333425199e72de6ea7fd2d6f59b46a2ac5cb5a85","observation_id":"4f42f8de-f2ee-4a8c-a8d5-c2da2069c6ca","resolution":{"observed_at":"2026-08-10T18:51:26.983887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.987718Z","title":"2019, Science China Physics, Mechanics, and Astronomy, 62, 959508, doi: 10.1007/s11433-018-9354-y","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.987718Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:6e1b45dca8e7ff4d2fa594c735d0e2a654d598ea80c7c5e7eaf42c6ab04394a7","observation_id":"37571d37-4f3c-40a7-bfdb-75188df76365","resolution":{"observed_at":"2026-08-10T18:51:26.987718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.991629Z","title":"M., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.991629Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:88c3b038dea52898b7b2806cd42431a9c99505a4eb24f014420c1d8db397dbde","observation_id":"f2462ae1-2e2f-4de5-a50e-35e10bac868f","resolution":{"observed_at":"2026-08-10T18:51:26.991629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.995573Z","title":"A., Torres, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.995573Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:16f95ea65577a838c006a2a05220d5482c988b6bc4326119eff79faa2732b5f6","observation_id":"f0b6a406-a195-49a1-82e8-7ab05cb5ced0","resolution":{"observed_at":"2026-08-10T18:51:26.995573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:26.999395Z","title":"V., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:26.999395Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:83330ad99b78925e83e42cf376b7895d91d5ada3cb8698394104071a3c71144c","observation_id":"d303d4fb-d107-4cb8-800e-76beb0d94894","resolution":{"observed_at":"2026-08-10T18:51:26.999395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.003018Z","title":"2018, A&A, 615, A73, doi: 10.1051/0004-6361/201732408","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.003018Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:1f15ec9707a8b0bbdb064c599a7b2fc741902bbf2f769fba057e79fc0f78686c","observation_id":"02a046a0-e854-49c3-83e3-4fa5cbc6084b","resolution":{"observed_at":"2026-08-10T18:51:27.003018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.006357Z","title":"2022, MNRAS, 513, 3113, doi: 10.1093/mnras/stac1130","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.006357Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:cec33f8a8d61e65ecd01399fabedccc6a3243aefd919df01ea38d638b26c7b4d","observation_id":"2cdfc4ec-95c1-4de1-8cf5-2aabecee166d","resolution":{"observed_at":"2026-08-10T18:51:27.006357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201935485","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.258804Z","title":"2019, A&A, 627, A69, doi: 10.1051/0004-6361/201935485","venue":null,"work_id":"c55f166d-7652-4b61-b668-d6277fc7c695","year":2019},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.010022Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:6699f432af7216964a09b529016359eea9a4ecdd47fbd72cf06ad62f064558c6","observation_id":"929e07aa-de1d-4611-880a-b2b259d35917","resolution":{"observed_at":"2026-08-10T18:51:27.263834Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11132","last_updated":"2023-07-20T16:23:37Z","snapshot_observed_at":"2026-08-13T10:51:03.892815Z","submitted_at":"2023-07-20T16:23:37Z","title":"The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.11132","snapshot_observed_at":"2026-08-10T18:51:27.013581Z","title":"A., Bruel, P., Clark, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.013581Z"},"links":{"cited_paper":"/paper/2307.11132","citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:a58a712786985cdf98caebafb976de5cd18c8bd786eb32ae042a95094c3bb501","observation_id":"cfe5ee02-823f-4ad9-bb67-93fae1416f71","resolution":{"observed_at":"2026-08-10T18:51:27.013581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stad2159","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.235916Z","title":"Q., Han, J","venue":null,"work_id":"91cfedb6-4ca4-4333-8cb2-9f6e3eb5b0b5","year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.017775Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:c6b54c342771f820529ed2425f981504002a3b27a726552cb8c366cc5b21a2f8","observation_id":"651e34df-18cd-4b2d-a9c0-2e950325a101","resolution":{"observed_at":"2026-08-10T18:51:27.239792Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/745/1/100","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.223095Z","title":"S., & Taam, R","venue":null,"work_id":"4942fbda-f655-4389-9e25-f36c00938fa6","year":2012},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.021315Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:91af61b5cba1dee261300b48a775e48ea4d0535958211b1f780b99358740f15e","observation_id":"cf3adee2-f164-49d2-914d-62ce01227fe7","resolution":{"observed_at":"2026-08-10T18:51:27.227044Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stac2164","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.211514Z","title":"A., & Zyuzin, D","venue":null,"work_id":"5d1f5736-78e7-42a7-83b8-5e837fdefa4e","year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.025015Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d837644032645b875ee94cbe7b3e318780d30c1481fcf20b859325d290ac9934","observation_id":"5cbee43e-523b-4d86-b7ae-da88a0b7c642","resolution":{"observed_at":"2026-08-10T18:51:27.215422Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/306038","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.200466Z","title":"1998, ApJ, 503, 843, doi: 10.1086/306038","venue":null,"work_id":"268dd42a-e4a2-4900-a166-db56bcf67d68","year":1998},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.028603Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:6637dc5327d164eca7ac297ecdf913e94968ba511d492dc0e584fd4f1c427ba0","observation_id":"a3ef16e2-2897-45bc-829b-04d6fd253ef9","resolution":{"observed_at":"2026-08-10T18:51:27.204240Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.032406Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.032406Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:5b93c5a09f9aba643c6c02434bd32e8fa3719cdd06b69f3e551e59595f6f85e9","observation_id":"b113b35c-9f34-43ff-84f8-3cfd044d0418","resolution":{"observed_at":"2026-08-10T18:51:27.032406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/727/2/131","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.182263Z","title":"2011, ApJ, 727, 131, doi: 10.1088/0004-637X/727/2/131","venue":null,"work_id":"8bf108bb-134a-45eb-8538-f3a912bc49e0","year":2011},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.035901Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:e8224cde02801b9a28a4abae9de00a030a3a36f5904f991a58a2e1360190657e","observation_id":"4b0e3218-a73c-484a-baa7-55b2eec3d5f5","resolution":{"observed_at":"2026-08-10T18:51:27.186230Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.039586Z","title":"A., Coriat, M., Traulsen, I., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.039586Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:912ec0308c7a81405c55b7f8da6e1d9dfb2e5a8222a4149cec271c432cf97c1d","observation_id":"0b4b06a3-a069-4e34-aa01-9304ec9a10bc","resolution":{"observed_at":"2026-08-10T18:51:27.039586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.043036Z","title":"2022, Nature Astronomy, 6, 698, doi: 10.1038/s41550-022-01630-1","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.043036Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:9b72c509b3858887cbbd5fedc09a00895dc114c37e82ab058697215a57b266a3","observation_id":"80efa511-c743-4cf6-992b-9ade1dbabb15","resolution":{"observed_at":"2026-08-10T18:51:27.043036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.046830Z","title":"D., Yuan, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.046830Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:da61c8919fd4b7d36194918d622ecb299b12cab0dc548bebcd913e30c6863323","observation_id":"4b5147fd-7130-4f14-ba7e-44d288957bef","resolution":{"observed_at":"2026-08-10T18:51:27.046830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.050430Z","title":"M., Manchester, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.050430Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d41cc6df63f99e1fb1ace903df208abd14ee9c36c1f96f4549178df30e5298fb","observation_id":"1956fec3-bcf0-4c8c-83bb-035ea9451cba","resolution":{"observed_at":"2026-08-10T18:51:27.050430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20021570","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.145614Z","title":null,"venue":null,"work_id":"051a00aa-5b98-40db-95e5-87cccc8167e1","year":2003},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.053949Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:d7e07822363d1c2ab02614a22069b76b6f974b6f30265b7a312d226c6a072795","observation_id":"9768febd-04d9-4eaa-b394-d8f0b8c1c744","resolution":{"observed_at":"2026-08-10T18:51:27.149453Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.057318Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.057318Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:39afbbf60d15939ba46812d82eb7186fc5263fc84b92cccf9b6fe273a8992c76","observation_id":"3875de3f-ed15-4881-a398-37235e1cf3a0","resolution":{"observed_at":"2026-08-10T18:51:27.057318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ace10b","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.126905Z","title":"2023, ApJ, 952, 158, doi: 10.3847/1538-4357/ace10b","venue":null,"work_id":"b552f5c0-ec1c-4894-b684-b031beb286df","year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.060984Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:fa3ccf1c84140ebcad0a80aba9fa9d8670f843ac6290840cda1874b6cb90953d","observation_id":"6d1c0c74-4e58-4d81-84bf-7cbe7a4034f7","resolution":{"observed_at":"2026-08-10T18:51:27.130555Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.064573Z","title":"J., Han, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.064573Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:b61b4ba93222bef8ed19331218debab72f607009049da5ef7ce6e604905d080a","observation_id":"9a016db7-facc-4ccd-97c0-d50985e449ce","resolution":{"observed_at":"2026-08-10T18:51:27.064573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.068174Z","title":"A., Karpova, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.068174Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:f2044ce0767f21cacc2049e231266595c44a31a1eefea5d9d69b5c0d0eac61d6","observation_id":"43181f3c-b505-4aa0-9f5d-0c4ef65a2260","resolution":{"observed_at":"2026-08-10T18:51:27.068174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa3991","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T18:51:27.099615Z","title":"A., Karpova, A","venue":null,"work_id":"7b8365eb-2a20-4b31-b0d6-027bf122ea61","year":2021},"citing_paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-10T18:51:27.071611Z"},"links":{"citing_paper":"/paper/2501.10999"},"observation_digest":"sha256:97107752ed174e70194082e2b214abb024b191c096f41918a2d1876bf5d5f81a","observation_id":"afcd41d9-7aa1-4c30-bb2f-d32a7aa0756c","resolution":{"observed_at":"2026-08-10T18:51:27.104494Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.10999","last_updated":"2025-03-31T11:57:15Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-10T18:41:47.840505Z","submitted_at":"2025-01-19T10:04:00Z","title":"A new X-ray census of rotation powered pulsars"},"reference_resolution":{"displayed":83,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":53,"verified_exact":28,"verified_fuzzy":1},"total_outbound_references":83},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 83 of 83 outbound references and 0 inbound Pith citation observations for arXiv:2501.10999."}