{"as_of":"2026-08-18T09:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3fcf8118bf87b78e005f041b7f6856fb886719bde7e6985490530ad54c0f38e0","coverage":[{"denominator":79,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":79,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T11:20:40.100123Z","state":"measured"},{"denominator":79,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":79,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+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/2509.03001/citation-record","integrity":"/paper/2509.03001/integrity","json":"/paper/2509.03001/citation-record.json","paper":"/paper/2509.03001"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:20:31.250294Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.250294Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:95e12865e95e45d103339f4920fc92fc23f5ec9b57417db351d23ee8180bc3e8","observation_id":"0b99aa56-d7e6-4b9e-b3f6-935e3becd0ff","resolution":{"observed_at":"2026-08-05T11:20:31.250294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04331","last_updated":"2024-02-06T19:16:00Z","snapshot_observed_at":"2026-08-16T14:20:52.764347Z","submitted_at":"2024-02-06T19:16:00Z","title":"Spin evolution of neutron stars","version":1},"cited_work":{"arxiv_id":"2402.04331","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.04331","snapshot_observed_at":"2026-08-05T11:20:44.211160Z","title":"Spin evolution of neutron stars","venue":"astro-ph.HE","work_id":"7c91a3ab-2948-4f3b-9be4-ba4a34d8ee69","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.319247Z"},"links":{"cited_paper":"/paper/2402.04331","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:79afe2ec74f092d045fecc59f747074e77af82a25f818aabdc5501cc08dcfe66","observation_id":"9dfd1ca2-0a91-414f-a754-bd82d1dd603e","resolution":{"observed_at":"2026-08-05T11:20:44.215819Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.14844","last_updated":"2024-01-19T11:39:29Z","snapshot_observed_at":"2026-08-16T14:49:46.909293Z","submitted_at":"2023-10-23T12:09:06Z","title":"Early Accretion Onset in Long-Period Isolated Pulsars","version":2},"cited_work":{"arxiv_id":"2310.14844","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.14844","snapshot_observed_at":"2026-08-05T11:20:44.190105Z","title":"Early Accretion Onset in Long-Period Isolated Pulsars","venue":"astro-ph.HE","work_id":"d70c9a14-75da-4c91-a34f-ad4fbc9e20fc","year":2023},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.417227Z"},"links":{"cited_paper":"/paper/2310.14844","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:8bf452c4d1642c954ed2fe2e8ff8a1947d7e93924060701d9779ae514213ee6a","observation_id":"0f1b1a04-d216-48f0-a197-eafdda9e28cf","resolution":{"observed_at":"2026-08-05T11:20:44.194736Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10404","last_updated":"2020-01-28T15:15:59Z","snapshot_observed_at":"2026-08-14T00:24:03.755329Z","submitted_at":"2020-01-28T15:15:59Z","title":"The Impact of Metallicity on the Evolution of Rotation and Magnetic Activity of Sun-Like Stars","version":1},"cited_work":{"arxiv_id":"2001.10404","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.10404","snapshot_observed_at":"2026-08-05T11:20:44.168323Z","title":"The Impact of Metallicity on the Evolution of Rotation and Magnetic Activity of Sun-Like Stars","venue":"astro-ph.SR","work_id":"486740e9-c0e8-485e-a534-e1032f66e2b2","year":2020},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.612685Z"},"links":{"cited_paper":"/paper/2001.10404","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d32ad3c6619c4229610bbe8550cd33b5ace892331513ef26f6cad47692114ffd","observation_id":"9816da09-b5b7-4cd2-ab4b-dab1d1cbd710","resolution":{"observed_at":"2026-08-05T11:20:44.173840Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.06468","last_updated":"2025-05-09T23:43:36Z","snapshot_observed_at":"2026-08-18T03:09:34.426092Z","submitted_at":"2025-05-09T23:43:36Z","title":"Submillimeter observations of the white dwarf pulsar AR Sco","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.06468","snapshot_observed_at":"2026-08-05T11:20:31.728156Z","title":", author Gurwell , M.A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.728156Z"},"links":{"cited_paper":"/paper/2505.06468","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:95cae5d1237f046193a77507a91d39176e5a1b382c2160c9f7da7fd94a1cb174","observation_id":"115e9260-9bd9-4ea5-81b5-717f9e0754a1","resolution":{"observed_at":"2026-08-05T11:20:31.728156Z","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":"2026-08-05T11:20:31.814397Z","title":", year 1990","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.814397Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5864d84c4b234ad2d05021e86c23824f39ba0a37e1a916bf7d3bb368fa89f536","observation_id":"e3f5823d-5c30-4cbf-81a6-1f683563541d","resolution":{"observed_at":"2026-08-05T11:20:31.814397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401067","last_updated":"2004-01-07T05:47:26Z","snapshot_observed_at":"2026-08-17T02:34:24.437751Z","submitted_at":"2004-01-07T05:47:26Z","title":"Multifrequency Observations of Radio Pulse Broadening and Constraints on Interstellar Electron Density Microstructure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401067","snapshot_observed_at":"2026-08-05T11:20:31.945001Z","title":", author Cordes , J.M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:31.945001Z"},"links":{"cited_paper":"/paper/astro-ph/0401067","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d61d25ba790e93a1e906e9b4af9e1ce0e5b85f7253a342a27b2e0033b05d39ae","observation_id":"ec1966ff-2e5e-4508-8fe6-09eb7c3ba7a1","resolution":{"observed_at":"2026-08-05T11:20:31.945001Z","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":"10.1086/185072","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Lamb , D.Q","venue":"The Astrophysical Journal","work_id":"f90a4bd0-8607-4721-85cb-e7b8a4835bcc","year":1987},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.075075Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:58f5ac90b4fbd17dd28207f20aa4c52277fdd44b70fcd5e7f206b28570396304","observation_id":"0accdeeb-a49b-432d-a3d4-a8e69b275a52","resolution":{"observed_at":"2026-08-05T11:20:42.360942Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08131","last_updated":"2021-01-19T13:55:14Z","snapshot_observed_at":"2026-08-16T18:51:23.484357Z","submitted_at":"2021-01-19T13:55:14Z","title":"Pulse energy distribution for RRAT J0139+33 according to observations at the frequency 111 MHz","version":1},"cited_work":{"arxiv_id":"2101.08131","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08131","snapshot_observed_at":"2026-08-05T11:20:44.106339Z","title":"Pulse energy distribution for RRAT J0139+33 according to observations at the frequency 111 MHz","venue":"astro-ph.HE","work_id":"31555e09-7f4b-4fe4-8441-ae60d8358f20","year":2021},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.224355Z"},"links":{"cited_paper":"/paper/2101.08131","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:2c336e539dbf4bb5307d66e52e35b74a67d22a465868f3eadc69356f38408c2d","observation_id":"26a6ea9a-632f-4722-8bf7-70249afe67c8","resolution":{"observed_at":"2026-08-05T11:20:44.112053Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.20455","last_updated":"2025-06-25T14:04:54Z","snapshot_observed_at":"2026-08-17T16:58:00.744997Z","submitted_at":"2025-06-25T14:04:54Z","title":"A Sibling of AR Scorpii: SDSS J230641.47$+$244055.8 and the Observational Blueprint of White Dwarf Pulsars","version":1},"cited_work":{"arxiv_id":"2506.20455","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.20455","snapshot_observed_at":"2026-08-05T11:20:44.082628Z","title":"A Sibling of AR Scorpii: SDSS J230641.47$+$244055.8 and the Observational Blueprint of White Dwarf Pulsars","venue":"astro-ph.SR","work_id":"15aa3246-084b-4658-ab3b-42625517c0c6","year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.355833Z"},"links":{"cited_paper":"/paper/2506.20455","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ba3ca43fa3b23a28db900c4aae0564ed2c2e1a92d2fa64d986dcf499e0a141cb","observation_id":"fb57de60-e337-4da4-832f-3b7f839ec1ae","resolution":{"observed_at":"2026-08-05T11:20:44.087632Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-05T11:20:32.427683Z","title":", author Cromartie , H.T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.427683Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:66bbd71c69069015d355e1142e0cb8a2ed8be9a862fd196bfb83093b623c272e","observation_id":"cd521420-bd53-4235-b962-2a11cc597e22","resolution":{"observed_at":"2026-08-05T11:20:32.427683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.21805","last_updated":"2026-07-27T07:51:38Z","snapshot_observed_at":"2026-08-17T15:31:17.540830Z","submitted_at":"2025-08-29T17:38:02Z","title":"Gaia's promise to detect compact-object binaries: where we stand with the third data release","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.21805","snapshot_observed_at":"2026-08-05T11:20:32.494007Z","title":", author Chatterjee , S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.494007Z"},"links":{"cited_paper":"/paper/2508.21805","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:1469549e22093bdf5ecdbf254a34619b711c73d7348a9e1444058f0b93effde2","observation_id":"31b0a78b-d85a-4180-83dd-59ea7edce493","resolution":{"observed_at":"2026-08-05T11:20:32.494007Z","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":"2026-08-05T11:20:32.572838Z","title":", author Lazio , T.J.W","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.572838Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:2b74c1f4d3c1a54f5d8f2d18d37d0f448c86932e70e533a0b87d5975a66298ca","observation_id":"faa1d726-e6ad-426a-a905-47adf7c05e0b","resolution":{"observed_at":"2026-08-05T11:20:32.572838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.13660","last_updated":"2025-06-16T16:19:42Z","snapshot_observed_at":"2026-08-18T04:51:04.671537Z","submitted_at":"2025-06-16T16:19:42Z","title":"Supernova explosions of runaway stars and young neutron stars above the Galactic plane","version":1},"cited_work":{"arxiv_id":"2506.13660","doi":"10.48550/arxiv.2506.13660","metadata_source":"pith","pith_arxiv_id":"2506.13660","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Supernova explosions of runaway stars and young neutron stars above the Galactic plane","venue":"astro-ph.SR","work_id":"f0a02ed5-a206-4fbb-8c93-f09c55db82b6","year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.694056Z"},"links":{"cited_paper":"/paper/2506.13660","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:93a4935b183efe754c70c0ae7af5d4452a5c84d8c8075aa2fa54916ec33abc1e","observation_id":"6c399e85-fc9e-4d12-a990-c7f14d6d12d4","resolution":{"observed_at":"2026-08-05T11:20:41.750261Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-05T11:20:32.848393Z","title":", author Rajwade , K.M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.848393Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:714a5538560403b5e940006d76a8f170d4141d573046598f5b05fc6ce41423fb","observation_id":"bc7681dc-e782-46c3-81a3-ead53c4f4080","resolution":{"observed_at":"2026-08-05T11:20:32.848393Z","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":"2026-08-05T11:20:44.272110Z","title":", year 1983","venue":null,"work_id":"a07e772c-42b3-4189-8661-6e90c38d189f","year":1983},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:32.969597Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:c8d5a13d84f2b36b6a96c76a42dfb4ae2772a605f43dde60098671fecb5a30f5","observation_id":"5321ef0f-abc3-4f76-acf3-3b7c38e7e360","resolution":{"observed_at":"2026-08-05T11:20:44.276522Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.12146","last_updated":"2024-05-14T15:07:26Z","snapshot_observed_at":"2026-08-16T14:08:39.864243Z","submitted_at":"2024-03-18T18:02:11Z","title":"Gaia's binary star renaissance","version":2},"cited_work":{"arxiv_id":"2403.12146","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.12146","snapshot_observed_at":"2026-08-05T11:20:44.044841Z","title":"Gaia's binary star renaissance","venue":"astro-ph.SR","work_id":"28f411ae-ed0d-4183-ad4d-764327ee5534","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.041393Z"},"links":{"cited_paper":"/paper/2403.12146","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:57375ad02b360487cb1761b8de356ab6f24f5bc0af86cb4f87c1c1d8ee41fcac","observation_id":"4c2ed7a8-ea36-4081-8fe5-4981961c7127","resolution":{"observed_at":"2026-08-05T11:20:44.049922Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:20:44.256049Z","title":", author Rix , H.W","venue":null,"work_id":"bc26f52d-2790-45ba-8fe9-746f1d4bbb31","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.191994Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d603c602b034f3513faa17061e1eaeb4bdc4d2176663f4a47970ec49427d2cb7","observation_id":"c5602f68-c32c-4250-a6a3-237e85652b8c","resolution":{"observed_at":"2026-08-05T11:20:44.261089Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2508.11462","last_updated":"2025-08-15T13:24:05Z","snapshot_observed_at":"2026-08-08T07:12:24.685281Z","submitted_at":"2025-08-15T13:24:05Z","title":"Search of RRATs on declinations from $+42^{\\circ}$ to $+55^{\\circ}$ with a neural network","version":1},"cited_work":{"arxiv_id":"2508.11462","doi":null,"metadata_source":"pith","pith_arxiv_id":"2508.11462","snapshot_observed_at":"2026-08-05T11:20:44.023401Z","title":"Search of RRATs on declinations from $+42^{\\circ}$ to $+55^{\\circ}$ with a neural network","venue":"astro-ph.HE","work_id":"7d8723d9-5288-4d87-abee-09256e3e2072","year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.347093Z"},"links":{"cited_paper":"/paper/2508.11462","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:c93a6e35401238a1b946396823342caf55641277cc8c6dfdee09f0662a1a1f5d","observation_id":"12fd2b17-d869-4a89-950b-29e2455ac452","resolution":{"observed_at":"2026-08-05T11:20:44.028091Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.08377","last_updated":"2021-06-13T17:11:48Z","snapshot_observed_at":"2026-08-16T18:45:08.109240Z","submitted_at":"2021-02-16T18:59:59Z","title":"Confirmation of a Second Propeller: A High-Inclination Twin of AE~Aquarii","version":2},"cited_work":{"arxiv_id":"2102.08377","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.08377","snapshot_observed_at":"2026-08-05T11:20:44.000937Z","title":"Confirmation of a Second Propeller: A High-Inclination Twin of AE~Aquarii","venue":"astro-ph.SR","work_id":"f786f7ca-3d77-4d25-a6c1-d846d66b8b28","year":2021},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.507840Z"},"links":{"cited_paper":"/paper/2102.08377","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:7500ce16a8f750811551edf0437ae51e4960997bf01003d4a6bb78c00d5f690b","observation_id":"8ae3b3ce-0a89-4c1e-bec2-4a01b5bc19e8","resolution":{"observed_at":"2026-08-05T11:20:44.006476Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04520","last_updated":"2019-01-14T19:08:51Z","snapshot_observed_at":"2026-08-14T17:31:06.762677Z","submitted_at":"2019-01-14T19:08:51Z","title":"astroquery: An Astronomical Web-Querying Package in Python","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.04520","snapshot_observed_at":"2026-08-05T11:20:33.611191Z","title":", author Sip o cz , B.M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.611191Z"},"links":{"cited_paper":"/paper/1901.04520","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ee9db67cc9b5965c5d155024b0f18104625686444af6fdc1d235e74e03a6e0f4","observation_id":"31c01e1a-df0a-44ef-9694-04a6951ddb3b","resolution":{"observed_at":"2026-08-05T11:20:33.611191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1593","last_updated":"2009-01-12T15:21:28Z","snapshot_observed_at":"2026-08-15T16:46:24.368319Z","submitted_at":"2009-01-12T15:21:28Z","title":"Pulsars as Fantastic Objects and Probes","version":1},"cited_work":{"arxiv_id":"0901.1593","doi":null,"metadata_source":"pith","pith_arxiv_id":"0901.1593","snapshot_observed_at":"2026-08-05T11:20:43.960842Z","title":"Pulsars as Fantastic Objects and Probes","venue":"astro-ph.SR","work_id":"106eb6cd-89b4-4937-b30e-718c35a00918","year":2009},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.718930Z"},"links":{"cited_paper":"/paper/0901.1593","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ee1a2607cd3dd62553e61d13199bcc5b4b451d1f86090dd00cf6f025c2316b3e","observation_id":"1256c1cb-f98b-4bda-bfe1-2be767fbb419","resolution":{"observed_at":"2026-08-05T11:20:43.965835Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07332","last_updated":"2019-06-18T01:35:24Z","snapshot_observed_at":"2026-08-14T16:14:13.777889Z","submitted_at":"2019-06-18T01:35:24Z","title":"Bo\\\"otes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem","version":1},"cited_work":{"arxiv_id":"1906.07332","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.07332","snapshot_observed_at":"2026-08-05T11:20:43.935983Z","title":"Bo\\\"otes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem","venue":"astro-ph.GA","work_id":"36c15452-7b11-43f2-ae1a-a218e4225825","year":2019},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:33.895458Z"},"links":{"cited_paper":"/paper/1906.07332","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:996994b401910a1fd57f70ff5e2a44f33de3f89b12629c3f61d9f01f97a0e683","observation_id":"72656d10-bc55-4341-93a4-db191e3fbfd6","resolution":{"observed_at":"2026-08-05T11:20:43.941299Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.15757","last_updated":"2024-11-25T07:54:27Z","snapshot_observed_at":"2026-08-16T13:23:13.186100Z","submitted_at":"2024-08-28T12:49:51Z","title":"A 2.9-hour periodic radio transient with an optical counterpart","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.15757","snapshot_observed_at":"2026-08-05T11:20:34.032787Z","title":", author McSweeney , S.J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.032787Z"},"links":{"cited_paper":"/paper/2408.15757","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:cd027f5310865ea5650f54765a423dc924dba33ed2cb2622218004e04250b14d","observation_id":"4b7bdcd1-e125-49df-8e71-70869538de38","resolution":{"observed_at":"2026-08-05T11:20:34.032787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.07494","last_updated":"2015-05-19T22:49:10Z","snapshot_observed_at":"2026-08-14T22:54:55.698830Z","submitted_at":"2015-03-25T18:59:12Z","title":"Stellar Winds on the Main-Sequence II: the Evolution of Rotation and Winds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.07494","snapshot_observed_at":"2026-08-05T11:20:34.178282Z","title":"u del , M. , author Brott , I. , author L \\","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.178282Z"},"links":{"cited_paper":"/paper/1503.07494","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:91b4d831a24b88064985bac678fa88fff0eb19e7dece159d87443b8aba9f5e60","observation_id":"86656575-f227-481a-bc4d-32838476c13f","resolution":{"observed_at":"2026-08-05T11:20:34.178282Z","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":"10.5281/zenodo.6390905","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", year 2022","venue":"Zenodo (CERN European Organization for Nuclear Research)","work_id":"dc913206-c6fb-4b93-bd97-d270cca498a1","year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.285430Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5679f46c232b7a39508256d4d7044466219259e3d6a1b692ccf31cac575cd809","observation_id":"34146883-9ecb-4848-9285-91a29c51243e","resolution":{"observed_at":"2026-08-05T11:20:41.562118Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1109.6896","last_updated":"2011-09-30T16:54:25Z","snapshot_observed_at":"2026-08-15T09:25:47.006365Z","submitted_at":"2011-09-30T16:54:25Z","title":"Rotating Radio Transients","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.6896","snapshot_observed_at":"2026-08-05T11:20:34.411640Z","title":", author McLaughlin , M.A","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.411640Z"},"links":{"cited_paper":"/paper/1109.6896","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:cfc2a5f2c99a052fe9eac558d6fd4ce6a390df6603d625368bde10304c9e5b4a","observation_id":"6f8a75cf-d1ac-47ff-adc8-7a3a7b5259fa","resolution":{"observed_at":"2026-08-05T11:20:34.411640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07885","last_updated":"2024-02-12T18:50:10Z","snapshot_observed_at":"2026-08-16T14:19:14.126897Z","submitted_at":"2024-02-12T18:50:10Z","title":"Stellar flares","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07885","snapshot_observed_at":"2026-08-05T11:20:34.549133Z","title":", year 2024","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.549133Z"},"links":{"cited_paper":"/paper/2402.07885","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5cfb24fdbf5f14060e4014d3d8ba30a9346dbdeae6d510ad14595a362bc0bbad","observation_id":"3193a567-384b-4e26-8bd1-3b90dd822e61","resolution":{"observed_at":"2026-08-05T11:20:34.549133Z","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":"10.1134/s1063772907080021","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Losovskii , B.Y","venue":"Astronomy Reports","work_id":"8431fee0-a4e4-44b5-86bd-74dcc1b2b85a","year":2007},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.655471Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:bc134dbf9df54e4925c635118b2c164e343f9e53f6bed61acf93f91a1f7feac0","observation_id":"11ce9516-7ca5-44ae-9d7a-9e73aac936a2","resolution":{"observed_at":"2026-08-05T11:20:41.361051Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1808.02035","last_updated":"2019-09-27T18:00:00Z","snapshot_observed_at":"2026-08-17T12:03:23.585764Z","submitted_at":"2018-08-06T18:00:02Z","title":"Mid-Infrared Spectroscopic Evidence for AGN Heating Warm Molecular Gas","version":2},"cited_work":{"arxiv_id":"1808.02035","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.02035","snapshot_observed_at":"2026-08-05T11:20:43.863147Z","title":"Mid-Infrared Spectroscopic Evidence for AGN Heating Warm Molecular Gas","venue":"astro-ph.GA","work_id":"76128cbb-0e54-463a-b844-0559cc26ce74","year":2018},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.773282Z"},"links":{"cited_paper":"/paper/1808.02035","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d27102108684d14ab5e1461aaead61b829a1cacdc093088c208f656ada34ac72","observation_id":"31539561-7306-4322-8d9a-9beeef4f7589","resolution":{"observed_at":"2026-08-05T11:20:43.867774Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-05T11:20:34.864231Z","title":", author Floyd , O","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.864231Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:8abc9369a9ef02f3b6e3f99bb1ae46f113ca432ccbf690925f090c5f28ebaaa9","observation_id":"0f16db6f-6e39-4c98-b352-d3551a5fa220","resolution":{"observed_at":"2026-08-05T11:20:34.864231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.11360","last_updated":"2023-02-10T10:07:37Z","snapshot_observed_at":"2026-08-16T16:22:30.397710Z","submitted_at":"2022-10-20T15:51:00Z","title":"An X-Ray-dim \"Isolated'' Neutron Star in a Binary?","version":4},"cited_work":{"arxiv_id":"2210.11360","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.11360","snapshot_observed_at":"2026-08-05T11:20:43.841293Z","title":"An X-Ray-dim \"Isolated'' Neutron Star in a Binary?","venue":"astro-ph.HE","work_id":"90d5b704-4547-4c9d-b9d0-5632cce0412b","year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:34.993046Z"},"links":{"cited_paper":"/paper/2210.11360","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:df085b84acbbb3f4a3c1296fc57afcd7f96c7c79f589ba37abfcf97c3566e254","observation_id":"2ed6ce3b-e84a-4d24-a972-343a0767f995","resolution":{"observed_at":"2026-08-05T11:20:43.846330Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:20:44.240776Z","title":", year 1992","venue":null,"work_id":"2631ba76-8536-497d-91e7-d9663b4c7f71","year":1992},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.127230Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:51dbbce3aa327c104ffe4ae416bb369991c24dcd9084c1ec98401ddc031cdc7c","observation_id":"c7681f66-86db-46a4-9576-38b94c9dbc36","resolution":{"observed_at":"2026-08-05T11:20:44.245108Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bf00651401","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Prokhorov , M.E","venue":"Astrophysics and Space Science","work_id":"8b823ace-3139-476e-a82e-1e6bb93957b2","year":1984},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.238991Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5306d4e795e9aa620c378d795f405cda6574576c757a52785ffe5b6962998d4a","observation_id":"28851af7-7648-46b4-8867-18802df63291","resolution":{"observed_at":"2026-08-05T11:20:41.155257Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.09825","last_updated":"2024-05-16T05:50:53Z","snapshot_observed_at":"2026-08-16T13:52:17.671420Z","submitted_at":"2024-05-16T05:50:53Z","title":"A Sample of Compact Object Candidates in Single-lined Spectroscopic Binaries from LAMOST Medium Resolution Survey","version":1},"cited_work":{"arxiv_id":"2405.09825","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.09825","snapshot_observed_at":"2026-08-05T11:20:43.818253Z","title":"A Sample of Compact Object Candidates in Single-lined Spectroscopic Binaries from LAMOST Medium Resolution Survey","venue":"astro-ph.SR","work_id":"68e4c4e1-e7a4-4e64-b7b3-1b7f01a833c6","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.351212Z"},"links":{"cited_paper":"/paper/2405.09825","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ec70cbcaa2a2dc30d131a265b736fe4cb885b5bf59173a1368338ee6f9b1c62b","observation_id":"2a5249cb-8aa4-44ae-b448-61a5b6244465","resolution":{"observed_at":"2026-08-05T11:20:43.823812Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.2419","last_updated":"2013-12-08T16:06:54Z","snapshot_observed_at":"2026-08-14T23:59:38.134345Z","submitted_at":"2013-10-09T09:59:52Z","title":"Fast radio bursts may originate from nearby flaring stars","version":3},"cited_work":{"arxiv_id":"1310.2419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.2419","snapshot_observed_at":"2026-08-05T11:20:43.796259Z","title":"Fast radio bursts may originate from nearby flaring stars","venue":"astro-ph.HE","work_id":"c8448667-d476-468a-8680-296f6b8dcbad","year":2013},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.467275Z"},"links":{"cited_paper":"/paper/1310.2419","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:e7a124f9a012de510dbbc2bb04f3f034091baf84bf819b583b6ad0c341acb260","observation_id":"1e3af767-7a46-41aa-ac9a-2ad200e7e041","resolution":{"observed_at":"2026-08-05T11:20:43.801015Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.00300","last_updated":"2023-01-18T20:52:56Z","snapshot_observed_at":"2026-08-18T08:49:03.003596Z","submitted_at":"2022-10-01T15:45:18Z","title":"Centrifugal barriers in magnetospheric accretion","version":3},"cited_work":{"arxiv_id":"2210.00300","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.00300","snapshot_observed_at":"2026-08-05T11:20:43.772951Z","title":"Centrifugal barriers in magnetospheric accretion","venue":"astro-ph.HE","work_id":"33c5dc81-25b9-4f12-93e9-ed9d17e8e1e1","year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.589941Z"},"links":{"cited_paper":"/paper/2210.00300","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:937836955205de5026b9c1e3e0f8938aba4d94ed34ac37e98f775af0381cce8c","observation_id":"1485ee72-9f81-49cd-8561-7cbf424854c5","resolution":{"observed_at":"2026-08-05T11:20:43.778089Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.22323/1.401.0046","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Meintjes , P","venue":null,"work_id":"a6ff0bd7-b6b1-47ef-82fb-634a81926eaa","year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.729478Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:10549acafa7ebc571a03ce25e90cfa2d8697a3ea68ad17abf974f569b712d4d0","observation_id":"d7d91bf4-d892-4676-bc24-3ed3839b9a9a","resolution":{"observed_at":"2026-08-05T11:20:40.991248Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08265","last_updated":"2016-07-27T21:16:18Z","snapshot_observed_at":"2026-08-15T14:40:37.792648Z","submitted_at":"2016-07-27T21:16:18Z","title":"A radio pulsing white dwarf binary star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.08265","snapshot_observed_at":"2026-08-05T11:20:35.814493Z","title":"a nsicke , B.T. , author H \\","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.814493Z"},"links":{"cited_paper":"/paper/1607.08265","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d4e76ff972259aa01a3c48399faec531325655abe15c42524a92be12bdf6f54c","observation_id":"d5997b3f-919a-458b-bfda-72daa8602382","resolution":{"observed_at":"2026-08-05T11:20:35.814493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.08618","last_updated":"2017-03-10T10:41:30Z","snapshot_observed_at":"2026-08-14T21:18:54.374907Z","submitted_at":"2017-01-30T14:34:46Z","title":"Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries","version":2},"cited_work":{"arxiv_id":"1701.08618","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.08618","snapshot_observed_at":"2026-08-05T11:20:43.734257Z","title":"Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries","venue":"astro-ph.HE","work_id":"0b587443-7edc-429a-860c-f373bad5aeb2","year":2017},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:35.925788Z"},"links":{"cited_paper":"/paper/1701.08618","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:eb6a940b04e4f9ca60cc08f92761f8a44366148b23c4d74b3d5b16c71297e50b","observation_id":"393036e5-4feb-46d1-8069-17806563ab86","resolution":{"observed_at":"2026-08-05T11:20:43.739083Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:20:44.226252Z","title":"a ttil \\","venue":null,"work_id":"69954980-f343-4479-aa57-4b0b51939d8f","year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.048597Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:afa8c602e827ed7bcf59783e3a8b4282f078a9c4e8c2c73bb16959ed78edcfe8","observation_id":"0db0dec0-329b-4ac7-9031-b6a81db8df66","resolution":{"observed_at":"2026-08-05T11:20:44.230566Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0907.2883","last_updated":"2009-07-16T16:49:20Z","snapshot_observed_at":"2026-08-15T19:13:44.346585Z","submitted_at":"2009-07-16T16:49:20Z","title":"Stellar wind accretion in high-mass X-ray binaries","version":1},"cited_work":{"arxiv_id":"0907.2883","doi":null,"metadata_source":"pith","pith_arxiv_id":"0907.2883","snapshot_observed_at":"2026-08-05T11:20:43.711689Z","title":"Stellar wind accretion in high-mass X-ray binaries","venue":"astro-ph.HE","work_id":"bd560ab0-3fb2-42ad-83c6-d096a5774d7e","year":2009},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.202052Z"},"links":{"cited_paper":"/paper/0907.2883","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:4c49799ab13ffaeaa49ddbdbf80d93304384bbc3e69f4a0bb4873600c39056ae","observation_id":"35efdbcb-cb34-4aca-a479-304895195509","resolution":{"observed_at":"2026-08-05T11:20:43.717111Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04674","last_updated":"2016-09-15T14:36:12Z","snapshot_observed_at":"2026-08-14T21:39:43.157102Z","submitted_at":"2016-09-15T14:36:12Z","title":"A Very Bright, Very Hot, and Very Long Flaring Event from the M Dwarf Binary System DG CVn","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.04674","snapshot_observed_at":"2026-08-05T11:20:36.338518Z","title":", author Kowalski , A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.338518Z"},"links":{"cited_paper":"/paper/1609.04674","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:541dc71250e230836b42c1076122afc983a7dd98a1e413b558f418ba45f0b0b8","observation_id":"10b83cd4-df77-413c-ac51-5bd7e9971abf","resolution":{"observed_at":"2026-08-05T11:20:36.338518Z","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":"2026-08-05T11:20:36.413692Z","title":", year 1994","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.413692Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5ee056ca82b8e5ff3c4d835876990c221909e9273430063ee6e98e5c0f19b6bc","observation_id":"3672f59c-2d21-4297-bccc-bccf10608e4d","resolution":{"observed_at":"2026-08-05T11:20:36.413692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.11015","last_updated":"2024-05-14T16:23:11Z","snapshot_observed_at":"2026-08-16T14:17:52.736544Z","submitted_at":"2024-02-16T19:00:04Z","title":"A Survey for Radio Emission from White Dwarfs in the VLA Sky Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.11015","snapshot_observed_at":"2026-08-05T11:20:36.501571Z","title":", author Chomiuk , L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.501571Z"},"links":{"cited_paper":"/paper/2402.11015","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ee95fe429c7a888c908bfeb5734ed7f0ccc9f20c8c96d0d581918a4c5a16fb3b","observation_id":"dfa2c16e-9f56-4cf0-803b-28362234e710","resolution":{"observed_at":"2026-08-05T11:20:36.501571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.09272","last_updated":"2023-06-15T16:49:03Z","snapshot_observed_at":"2026-08-16T15:23:35.665483Z","submitted_at":"2023-06-15T16:49:03Z","title":"A 5.3-minute-period pulsing white dwarf in a binary detected from radio to X-rays","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.09272","snapshot_observed_at":"2026-08-05T11:20:36.595062Z","title":", author Marsh , T.R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.595062Z"},"links":{"cited_paper":"/paper/2306.09272","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:6537781f68e99cf818e23e8d37228ee36c90f567d72883105d8f7a112bb5fd65","observation_id":"0f104e46-3469-4fa2-b9de-2132788a7364","resolution":{"observed_at":"2026-08-05T11:20:36.595062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.4587","last_updated":"2008-12-25T06:08:13Z","snapshot_observed_at":"2026-08-15T07:18:44.313294Z","submitted_at":"2008-12-25T06:08:13Z","title":"Scenarios for GCRT J1745-3009","version":1},"cited_work":{"arxiv_id":"0812.4587","doi":"10.48550/arxiv.0812.4587","metadata_source":"pith","pith_arxiv_id":"0812.4587","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Scenarios for GCRT J1745-3009","venue":"astro-ph","work_id":"532d2d8f-dda6-4ef7-b0d2-403d547c99f4","year":2008},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.712904Z"},"links":{"cited_paper":"/paper/0812.4587","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:2b4819b21a0ab9530b9247baf13fefa9bbe4508f4ad0d755c20bb7ba9d90cfd7","observation_id":"93b98e08-3030-4313-92df-b2accbbb89ff","resolution":{"observed_at":"2026-08-05T11:20:40.746318Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02084","last_updated":"2023-06-03T11:11:59Z","snapshot_observed_at":"2026-08-16T15:26:54.837241Z","submitted_at":"2023-06-03T11:11:59Z","title":"The zoo of isolated neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.02084","snapshot_observed_at":"2026-08-05T11:20:36.838962Z","title":", year 2023","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.838962Z"},"links":{"cited_paper":"/paper/2306.02084","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d62950b3901df4f6f09ef41ebac5a376a1a43adbb7fd9b72323d0b283b4f2f24","observation_id":"165270c8-89f8-434a-8bad-1c0f32dba4bb","resolution":{"observed_at":"2026-08-05T11:20:36.838962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.08800","last_updated":"2021-02-17T14:57:32Z","snapshot_observed_at":"2026-08-16T18:44:56.143014Z","submitted_at":"2021-02-17T14:57:32Z","title":"Radio and optical observations of the possible AE Aqr twin, LAMOST J024048.51+195226.9","version":1},"cited_work":{"arxiv_id":"2102.08800","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.08800","snapshot_observed_at":"2026-08-05T11:20:43.617340Z","title":"Radio and optical observations of the possible AE Aqr twin, LAMOST J024048.51+195226.9","venue":"astro-ph.SR","work_id":"7819fec0-dd75-4d20-b62a-a0dd80fba1a2","year":2021},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:36.901186Z"},"links":{"cited_paper":"/paper/2102.08800","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d45234852cd90c10a44ac9f40405651548f4d13e62aff49ff52d8e517ebdc9e7","observation_id":"180c1a8a-50bc-43e4-bf57-cc74e12e64d3","resolution":{"observed_at":"2026-08-05T11:20:43.624532Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.03315","last_updated":"2025-02-12T22:45:50Z","snapshot_observed_at":"2026-08-14T15:20:55.509459Z","submitted_at":"2025-01-06T19:00:01Z","title":"Spectroscopic Detection of a 2.9-hour Orbit in a Long Period Radio Transient","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.03315","snapshot_observed_at":"2026-08-05T11:20:37.060126Z","title":", year 2025","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.060126Z"},"links":{"cited_paper":"/paper/2501.03315","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ebbb75c4dfb4b7ac0b295210aac3f0ffbb0ac82a5f5d51e4f041edcb42335c9e","observation_id":"69422834-c802-449e-ae30-2cdaa700f86b","resolution":{"observed_at":"2026-08-05T11:20:37.060126Z","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":"10.1063/1.1419603","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Toropina , O.D","venue":"AIP conference proceedings","work_id":"843c6366-a4cc-402f-b0ab-0364d49ae14d","year":2001},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.185348Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:ada440c9c53562f38b9f20b151f8cb5e3d6d47161a21e5a4237e61631ac31852","observation_id":"778fdcd6-9e72-4657-9c48-d204955a3bed","resolution":{"observed_at":"2026-08-05T11:20:40.633125Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.12326","last_updated":"2023-11-12T23:50:06Z","snapshot_observed_at":"2026-08-16T15:22:12.193858Z","submitted_at":"2023-06-21T15:09:55Z","title":"What is the nature of the HESS J1731-347 compact object?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.12326","snapshot_observed_at":"2026-08-05T11:20:37.319403Z","title":", author Giangrandi , E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.319403Z"},"links":{"cited_paper":"/paper/2306.12326","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5181c4dd3db060fa6018ffd269ce074912e5ddc24c54570f0fe8b8530c4cbf15","observation_id":"d2a73921-d41d-44eb-92ec-a924e5f6eba9","resolution":{"observed_at":"2026-08-05T11:20:37.319403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3474","last_updated":"2012-11-15T01:23:07Z","snapshot_observed_at":"2026-08-15T16:48:04.338618Z","submitted_at":"2012-11-15T01:23:07Z","title":"A decade of solar Type III radio bursts observed by the Nancay Radioheliograph 1998-2008","version":1},"cited_work":{"arxiv_id":"1211.3474","doi":null,"metadata_source":"pith","pith_arxiv_id":"1211.3474","snapshot_observed_at":"2026-08-05T11:20:43.560690Z","title":"A decade of solar Type III radio bursts observed by the Nancay Radioheliograph 1998-2008","venue":"astro-ph.SR","work_id":"331eef8b-c7f5-4c0f-b7ad-ed646735041e","year":2012},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.429149Z"},"links":{"cited_paper":"/paper/1211.3474","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:5a614506e2bcb3aca41fb3dbeb24d113ba198b2e823caaa700125b61d1a00876","observation_id":"75b91a89-d6de-4d15-8d86-5cd1c9b1fbf0","resolution":{"observed_at":"2026-08-05T11:20:43.565460Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.14923","last_updated":"2024-11-20T16:53:28Z","snapshot_observed_at":"2026-08-16T22:15:15.605765Z","submitted_at":"2024-09-23T11:19:19Z","title":"A NICER View of PSR J1231$-$1411: A Complex Case","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.14923","snapshot_observed_at":"2026-08-05T11:20:37.535088Z","title":", author Deneva , J.S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.535088Z"},"links":{"cited_paper":"/paper/2409.14923","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:31993127607d5a577419508c2b4c34d5c9b03a4460d488e5977b755da4f88810","observation_id":"449dab62-d88d-4ac9-b314-9a80899bbdbb","resolution":{"observed_at":"2026-08-05T11:20:37.535088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.16170","last_updated":"2024-04-24T20:00:17Z","snapshot_observed_at":"2026-08-16T13:58:05.539372Z","submitted_at":"2024-04-24T20:00:17Z","title":"Swift X-Ray and UV Observations of six Gaia Binaries supposedly containing a Neutron Star","version":1},"cited_work":{"arxiv_id":"2404.16170","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.16170","snapshot_observed_at":"2026-08-05T11:20:43.517803Z","title":"Swift X-Ray and UV Observations of six Gaia Binaries supposedly containing a Neutron Star","venue":"astro-ph.HE","work_id":"5357ac93-1598-464d-b922-a7333af7f3ca","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.614037Z"},"links":{"cited_paper":"/paper/2404.16170","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:b9124352e01233d44483b7231f1b108a93d35bd8b69220f9e04d38d8ccffcee9","observation_id":"97e95ccd-6a1d-4779-b040-6a226e7a9d21","resolution":{"observed_at":"2026-08-05T11:20:43.522947Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.10868","last_updated":"2021-04-09T11:56:02Z","snapshot_observed_at":"2026-08-15T16:38:25.420637Z","submitted_at":"2020-06-18T21:57:50Z","title":"Weighing stars from birth to death: mass determination methods across the HRD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.10868","snapshot_observed_at":"2026-08-05T11:20:37.699875Z","title":", author Weiss , A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.699875Z"},"links":{"cited_paper":"/paper/2006.10868","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:30b6806c0934aef16c24dff47724d1470c53c41124df410f8f7f1258a6274ada","observation_id":"5761040a-e4ad-4748-98fb-5863964a70ef","resolution":{"observed_at":"2026-08-05T11:20:37.699875Z","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":"10.1134/s1063772916110068","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":", author Chashei , I.V","venue":"Astronomy Reports","work_id":"5c875546-e408-43db-b791-5d65cfc697eb","year":2016},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.831439Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:24bbf7cb2f60ff157cf0657523235f8214362993afa159c996edf4de850f69fb","observation_id":"85c6682d-5552-47d3-909d-44e818a14bde","resolution":{"observed_at":"2026-08-05T11:20:40.405812Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.04478","last_updated":"2018-01-18T12:17:12Z","snapshot_observed_at":"2026-08-14T20:24:28.137987Z","submitted_at":"2017-10-12T12:51:05Z","title":"Stellar Winds and Coronae of Low-mass Pop. II/III Stars","version":2},"cited_work":{"arxiv_id":"1710.04478","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.04478","snapshot_observed_at":"2026-08-05T11:20:43.477655Z","title":"Stellar Winds and Coronae of Low-mass Pop. II/III Stars","venue":"astro-ph.SR","work_id":"5d847152-3f2f-41f2-ada4-b46a8360203f","year":2017},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:37.924735Z"},"links":{"cited_paper":"/paper/1710.04478","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:416741ee7ff627aba68340301a0e0d7f49c05f49e0405d7df5e4eaf3182ccd8a","observation_id":"927864aa-f21d-41c8-be61-494f05db8389","resolution":{"observed_at":"2026-08-05T11:20:43.482599Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.12539","last_updated":"2025-04-17T00:03:37Z","snapshot_observed_at":"2026-08-17T01:32:10.402456Z","submitted_at":"2025-04-17T00:03:37Z","title":"The Intergalactic Medium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.12539","snapshot_observed_at":"2026-08-05T11:20:38.016392Z","title":", year 2025","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.016392Z"},"links":{"cited_paper":"/paper/2504.12539","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:98ec0848326b6c70655dafe171615e88ac3a59dede7c552573a4cfc1041dfc13","observation_id":"be78024f-9aeb-40c1-969a-fac9706dc679","resolution":{"observed_at":"2026-08-05T11:20:38.016392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105422","last_updated":"2001-05-23T22:24:59Z","snapshot_observed_at":"2026-08-15T06:20:17.399736Z","submitted_at":"2001-05-23T22:24:59Z","title":"Propagation of Magnetized Neutron Stars Through the Interstellar Medium","version":1},"cited_work":{"arxiv_id":"astro-ph/0105422","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0105422","snapshot_observed_at":"2026-08-05T11:20:43.456229Z","title":"Propagation of Magnetized Neutron Stars Through the Interstellar Medium","venue":"astro-ph","work_id":"ed9b9fe5-cfa4-49e2-aa1e-39ee92fd06e5","year":2001},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.119532Z"},"links":{"cited_paper":"/paper/astro-ph/0105422","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:2d5238bf151f5a1b2940a88e1ede596adb5c8b2e3a3a9c20210a779d5041d4b3","observation_id":"da2d4126-1714-4218-8f20-7697396502d8","resolution":{"observed_at":"2026-08-05T11:20:43.461283Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.08224","last_updated":"2025-01-14T16:07:10Z","snapshot_observed_at":"2026-08-15T07:46:12.291552Z","submitted_at":"2025-01-14T16:07:10Z","title":"Discovery of 26 new Galactic radio transients by MeerTRAP","version":1},"cited_work":{"arxiv_id":"2501.08224","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.08224","snapshot_observed_at":"2026-08-05T11:20:43.434849Z","title":"Discovery of 26 new Galactic radio transients by MeerTRAP","venue":"astro-ph.HE","work_id":"309f276f-ad8b-4545-8c71-2403e5dcece1","year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.208632Z"},"links":{"cited_paper":"/paper/2501.08224","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:b1f69127c0e7abb9a810382414fa794927e802affcc8ffaa157e0e078ae8705f","observation_id":"c7b19884-2349-4792-b22a-62656fdc5f95","resolution":{"observed_at":"2026-08-05T11:20:43.439877Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.05142","last_updated":"2024-01-10T13:20:45Z","snapshot_observed_at":"2026-08-18T01:50:52.070544Z","submitted_at":"2024-01-10T13:20:45Z","title":"Search for rotating radio transients in PUMPS","version":1},"cited_work":{"arxiv_id":"2401.05142","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.05142","snapshot_observed_at":"2026-08-05T11:20:43.413682Z","title":"Search for rotating radio transients in PUMPS","venue":"astro-ph.HE","work_id":"609ed0c8-0c7b-4914-b4ec-f920ed4a3696","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.331634Z"},"links":{"cited_paper":"/paper/2401.05142","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:9a41852fc9bb1167e050f396a449d52e02bd3ac1e5badda4b8a7bcfbf7e464ac","observation_id":"0e078384-839a-4195-a0d1-3f7dc7353f21","resolution":{"observed_at":"2026-08-05T11:20:43.418352Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.01285","last_updated":"2024-07-01T13:39:33Z","snapshot_observed_at":"2026-08-16T13:38:07.696510Z","submitted_at":"2024-07-01T13:39:33Z","title":"Search for rotating radio transients in monitoring data for three years","version":1},"cited_work":{"arxiv_id":"2407.01285","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.01285","snapshot_observed_at":"2026-08-05T11:20:43.391058Z","title":"Search for rotating radio transients in monitoring data for three years","venue":"astro-ph.HE","work_id":"047bfc3f-f423-420b-9efb-025af9339970","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.409516Z"},"links":{"cited_paper":"/paper/2407.01285","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:346ef5b16a44c457a7dfe0f87993e7632e231c8ebb8dce4ee4f39443fec772e5","observation_id":"bc578cf8-7b41-4e7b-adac-c584c023ed7a","resolution":{"observed_at":"2026-08-05T11:20:43.395981Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.15540","last_updated":"2022-03-29T13:25:05Z","snapshot_observed_at":"2026-08-16T17:10:56.357833Z","submitted_at":"2022-03-29T13:25:05Z","title":"Pushchino multibeam pulsar search: I. Targeted search of weak pulsars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.15540","snapshot_observed_at":"2026-08-05T11:20:38.490677Z","title":", author Kitaeva , M.A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.490677Z"},"links":{"cited_paper":"/paper/2203.15540","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:febb264790babc8fdc18d46b95529342159283b74d3909658ed3e4f4b75f907f","observation_id":"dd9661fc-9e07-46fe-b0ec-172d2865504a","resolution":{"observed_at":"2026-08-05T11:20:38.490677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.07565","last_updated":"2018-07-19T08:24:26Z","snapshot_observed_at":"2026-08-15T07:20:00.325201Z","submitted_at":"2018-07-19T08:24:26Z","title":"Detection of 25 new rotating radio transients at 111 MHz","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.07565","snapshot_observed_at":"2026-08-05T11:20:38.577780Z","title":", author Tyul'bashev , V.S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.577780Z"},"links":{"cited_paper":"/paper/1807.07565","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:2c74fcee5521cc074b5670fc7d60f5fec8a2dc90d8d63ebe194db64ecb26b27f","observation_id":"5ec8f6fd-df18-4d06-9363-79a206483026","resolution":{"observed_at":"2026-08-05T11:20:38.577780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.11032","last_updated":"2022-07-22T12:14:14Z","snapshot_observed_at":"2026-08-16T16:44:04.413276Z","submitted_at":"2022-07-22T12:14:14Z","title":"Detection of Five New RRATs at 111 MHz","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.11032","snapshot_observed_at":"2026-08-05T11:20:38.656723Z","title":", author Tyul'bashev , V.S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.656723Z"},"links":{"cited_paper":"/paper/2207.11032","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:9a9ac96f5a950aa9ffd65ba8f56994c65aae5ce03955a3513850817c994c19c2","observation_id":"c0879a57-f5d9-47e7-aff4-8941d4c49652","resolution":{"observed_at":"2026-08-05T11:20:38.656723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.08839","last_updated":"2022-08-18T14:12:01Z","snapshot_observed_at":"2026-08-16T16:38:23.764751Z","submitted_at":"2022-08-18T14:12:01Z","title":"Detection of new pulsars at the frequency 111 MHz","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.08839","snapshot_observed_at":"2026-08-05T11:20:38.769601Z","title":", author Tyul'bashev , V.S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.769601Z"},"links":{"cited_paper":"/paper/2208.08839","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:c35debd1e657b276a1258f52ec33d2d6e0ce7a0494e1ff1fb8303515f6d6c100","observation_id":"aec2be0c-88dc-4162-9090-b9d2ed4f150e","resolution":{"observed_at":"2026-08-05T11:20:38.769601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.15104","last_updated":"2025-04-21T13:53:41Z","snapshot_observed_at":"2026-08-17T05:41:35.802730Z","submitted_at":"2025-04-21T13:53:41Z","title":"Search for pulsars with periods of more than two seconds at declinations from +21$^o$ to +42$^o$","version":1},"cited_work":{"arxiv_id":"2504.15104","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.15104","snapshot_observed_at":"2026-08-05T11:20:43.298637Z","title":"Search for pulsars with periods of more than two seconds at declinations from +21$^o$ to +42$^o$","venue":"astro-ph.HE","work_id":"4970773f-1e34-4a06-81f2-c0c81e5ea5c4","year":2025},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:38.910183Z"},"links":{"cited_paper":"/paper/2504.15104","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:a51df791d22adfd922255a277922e767347e2fbf3fdad8e801b50d327f57b5ac","observation_id":"6e37d143-2947-4a6b-b163-5cd8d642cbc0","resolution":{"observed_at":"2026-08-05T11:20:43.303721Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.11882","last_updated":"2020-06-21T19:25:08Z","snapshot_observed_at":"2026-08-15T09:57:04.316070Z","submitted_at":"2020-06-21T19:25:08Z","title":"Prospects for radio detection of stellar plasma beams","version":1},"cited_work":{"arxiv_id":"2006.11882","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.11882","snapshot_observed_at":"2026-08-05T11:20:43.177867Z","title":"Prospects for radio detection of stellar plasma beams","venue":"astro-ph.SR","work_id":"c011ded6-a92e-477e-b5bc-62a59e9a2737","year":2020},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.045895Z"},"links":{"cited_paper":"/paper/2006.11882","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:7a2f2669ff57a7591e7fbca4531b69da6d4a8104a088c766c3b8a8f68b91c583","observation_id":"7a4646b4-3d9c-46e5-b04a-2af92f224d2f","resolution":{"observed_at":"2026-08-05T11:20:43.229681Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2103.15748","last_updated":"2021-03-29T16:43:24Z","snapshot_observed_at":"2026-08-16T18:35:30.111280Z","submitted_at":"2021-03-29T16:43:24Z","title":"The evolution of the solar wind","version":1},"cited_work":{"arxiv_id":"2103.15748","doi":null,"metadata_source":"pith","pith_arxiv_id":"2103.15748","snapshot_observed_at":"2026-08-05T11:20:43.038725Z","title":"The evolution of the solar wind","venue":"astro-ph.SR","work_id":"5826ecb8-5ed0-4edf-9d2d-22e250a69a82","year":2021},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.144145Z"},"links":{"cited_paper":"/paper/2103.15748","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:89229381c53a5ae13b2f5a61cde30f385e060981604269f992eccd3109c354d9","observation_id":"a358b75d-7cbc-4c02-873c-45ae2c411350","resolution":{"observed_at":"2026-08-05T11:20:43.086278Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.16606","last_updated":"2024-11-26T06:50:55Z","snapshot_observed_at":"2026-08-16T15:06:35.777855Z","submitted_at":"2024-11-25T17:41:54Z","title":"Detection of X-ray Emission from a Bright Long-Period Radio Transient","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.16606","snapshot_observed_at":"2026-08-05T11:20:39.229939Z","title":", author Rea , N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.229939Z"},"links":{"cited_paper":"/paper/2411.16606","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:c31b73e8c897fa843c85eb863790dfaffd88a91d90e251b7fdce459b4bea0dd9","observation_id":"31f43bc8-9030-4629-aad9-6efa7ad82179","resolution":{"observed_at":"2026-08-05T11:20:39.229939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0002110","last_updated":"2000-02-04T18:14:32Z","snapshot_observed_at":"2026-08-14T23:18:57.716430Z","submitted_at":"2000-02-04T18:14:32Z","title":"The SIMBAD astronomical database","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0002110","snapshot_observed_at":"2026-08-05T11:20:39.318917Z","title":", author Ochsenbein , F","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.318917Z"},"links":{"cited_paper":"/paper/astro-ph/0002110","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:7e83db8f3552db86aaed8b95469da3137f0119bf631d4fddccf61042dc5b92e1","observation_id":"082ff4ab-3d0f-4b64-9d58-3bf94fd0c645","resolution":{"observed_at":"2026-08-05T11:20:39.318917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.3852","last_updated":"2011-08-22T16:06:55Z","snapshot_observed_at":"2026-08-16T00:47:00.299639Z","submitted_at":"2011-08-18T20:21:31Z","title":"The COS-Halos Survey: Keck LRIS and Magellan MagE Optical Spectroscopy","version":2},"cited_work":{"arxiv_id":"1108.3852","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.3852","snapshot_observed_at":"2026-08-05T11:20:42.880632Z","title":"The COS-Halos Survey: Keck LRIS and Magellan MagE Optical Spectroscopy","venue":"astro-ph.CO","work_id":"060a40de-2357-48fc-ab5e-45e8c90823f9","year":2011},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.428402Z"},"links":{"cited_paper":"/paper/1108.3852","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:b268b4d91451b8e433fd8803b9cfa23b9139806278a322af32340c2d091b79d0","observation_id":"a2d07fd3-88da-44ee-88bc-b73143e319ce","resolution":{"observed_at":"2026-08-05T11:20:42.948558Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-05T11:20:39.529236Z","title":", author King , A.R","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.529236Z"},"links":{"citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:d6c094e09797d3a18e52938a3f3da95e3d7e7364e0a943d94cd07738f1343779","observation_id":"955e8232-c4fc-4330-a171-47bde6046022","resolution":{"observed_at":"2026-08-05T11:20:39.529236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-08-14T21:32:56.697557Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-05T11:20:39.665646Z","title":", author Manchester , R.N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.665646Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:632cd171d4586d50852c4911c21cf95c384110d2341f120bf0d8cfb9b931e896","observation_id":"6c64266f-e9e6-41c6-a5c1-6571360d8fc0","resolution":{"observed_at":"2026-08-05T11:20:39.665646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.07162","last_updated":"2023-12-12T10:56:31Z","snapshot_observed_at":"2026-08-16T14:35:33.108704Z","submitted_at":"2023-12-12T10:56:31Z","title":"Radio emission as a stellar activity indicator","version":1},"cited_work":{"arxiv_id":"2312.07162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.07162","snapshot_observed_at":"2026-08-05T11:20:42.709458Z","title":"Radio emission as a stellar activity indicator","venue":"astro-ph.SR","work_id":"e5983d9c-2e49-46ca-a6d3-e97a9eb54048","year":2023},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.800924Z"},"links":{"cited_paper":"/paper/2312.07162","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:da8432162c629ab5af2793fc9dfb77d80fb8239f43e0239dd409c37780fdfa43","observation_id":"22047b05-8768-4dff-8e9e-447207f6cced","resolution":{"observed_at":"2026-08-05T11:20:42.757996Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.13404","last_updated":"2022-03-25T01:12:29Z","snapshot_observed_at":"2026-08-16T17:11:56.302423Z","submitted_at":"2022-03-25T01:12:29Z","title":"Statistical Analysis of H I Profile Asymmetry and Shape for Nearby Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.13404","snapshot_observed_at":"2026-08-05T11:20:39.896474Z","title":", author Ho , L.C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.896474Z"},"links":{"cited_paper":"/paper/2203.13404","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:87e21629eabb7ef3cf3ec56e3e2c89b4bea956f51147df7a55fcb8d5f966bd5e","observation_id":"684a5c07-b6e9-47e5-9524-27209aff9601","resolution":{"observed_at":"2026-08-05T11:20:39.896474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.03500","last_updated":"2020-11-06T18:18:56Z","snapshot_observed_at":"2026-08-18T04:07:11.631955Z","submitted_at":"2020-11-06T18:18:56Z","title":"The Physical Mechanisms of Fast Radio Bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.03500","snapshot_observed_at":"2026-08-05T11:20:39.997832Z","title":", year 2020","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.997832Z"},"links":{"cited_paper":"/paper/2011.03500","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:3e369f9048d648bc8a3a30d85d4367a8b37a3e4d7c62499d6145973676607b19","observation_id":"88cb91cb-f1dc-4e3e-917e-ca2db8d6fec9","resolution":{"observed_at":"2026-08-05T11:20:39.997832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.08289","last_updated":"2024-01-16T11:34:58Z","snapshot_observed_at":"2026-08-16T14:27:10.322988Z","submitted_at":"2024-01-16T11:34:58Z","title":"The hidden companion in J1527: a 0.69 solar-mass white dwarf?","version":1},"cited_work":{"arxiv_id":"2401.08289","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.08289","snapshot_observed_at":"2026-08-05T11:20:42.497004Z","title":"The hidden companion in J1527: a 0.69 solar-mass white dwarf?","venue":"astro-ph.SR","work_id":"661e464e-fa1c-45d0-adb0-6126ced04aee","year":2024},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:40.100123Z"},"links":{"cited_paper":"/paper/2401.08289","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:dc223464a3dde8a25166d9a91e1c1f0b35223c8464e7913a19124f981e2fe770","observation_id":"3e18b1d8-c584-4d55-a946-c33a660b4754","resolution":{"observed_at":"2026-08-05T11:20:42.599878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-13T05:42:09.292668Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates"},"reference_resolution":{"displayed":79,"state_counts":{"malformed_identifier":0,"metadata_mismatch":19,"parse_uncertain":0,"unresolved":35,"verified_exact":21,"verified_fuzzy":4},"total_outbound_references":79},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 79 of 79 outbound references and 0 inbound Pith citation observations for arXiv:2509.03001."}