{"as_of":"2026-08-18T09:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3513feb5b9e7ccecc51b4580f4a436c14f6de5c68e859b6d42bddb87145604b0","coverage":[{"denominator":48,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":48,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:13:45.405677Z","state":"measured"},{"denominator":48,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":48,"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/2505.10460/citation-record","integrity":"/paper/2505.10460/integrity","json":"/paper/2505.10460/citation-record.json","paper":"/paper/2505.10460"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/716/2/1566","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:46.144214Z","title":"2010, ApJ, 716, 1566, doi: 10.1088/0004-637X/716/2/1566","venue":null,"work_id":"e40c3fc3-4633-473e-9b2c-8c6646718fd8","year":2010},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.425914Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:a71c0e08bcbc1e3ee2e2db9ee0b6ddad228088c838a162868bf1261ce7d24fed","observation_id":"7e365647-07be-4184-8358-df212f14198d","resolution":{"observed_at":"2026-08-15T21:13:46.230812Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.545322Z","title":"A., & Hawley, J","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.545322Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:e7ee16d53f211f421ac9dd6516142b91cc57a76247dab25a16d92ce5313e48fa","observation_id":"9fe3620c-be17-4ad0-92f2-e7ec612469d4","resolution":{"observed_at":"2026-08-15T21:13:44.545322Z","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":"2026-08-15T21:13:47.066455Z","title":"1950, Zeitschrift Naturforschung Teil A, 5, 65","venue":null,"work_id":"f928be36-8513-4e28-acc5-55a7b0c3820d","year":1950},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.595008Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:758ce01985efbe052f2bef2bb9002587dda35671de02a2462975aafa7ca30802","observation_id":"34463284-1e7c-46d3-ad08-e91fcf15ed41","resolution":{"observed_at":"2026-08-15T21:13:47.158729Z","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":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.600787Z","title":"S., & Blinnikov, S","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.600787Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:071b731a4a33f62e2b5b1f4767121f8110e475360bcffbc8ea783effe9b7fd21","observation_id":"1c5aac28-f805-47d7-a582-f62378747f2f","resolution":{"observed_at":"2026-08-15T21:13:44.600787Z","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":"10.1086/342876","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:46.122607Z","title":"S., Lovelace, R","venue":null,"work_id":"1bfb1dd5-7020-4520-b7ce-4452f2893c52","year":2002},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.605794Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:49cd30b0a195f9644dd8ce398230aeb1c5ec346b5479e86b839b8d1be2eceea0","observation_id":"00d1abec-c2ee-4cc3-9acc-e504ebd16c68","resolution":{"observed_at":"2026-08-15T21:13:46.127050Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.610348Z","title":"G., Wen, S., Stone, N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.610348Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:b7ad1fb98f12ac97a0f5ab318b6d6dab82ba153633b8ef68dd5fe42895115ca5","observation_id":"6ab34446-d3b4-46b9-b209-29dcdbac6857","resolution":{"observed_at":"2026-08-15T21:13:44.610348Z","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":"10.1086/524699","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:46.100678Z","title":"M., Contopoulos, I., & Kazanas, D","venue":null,"work_id":"2af04c96-74f1-44f5-b324-e7839c3d55aa","year":2008},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.619495Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:830146986729a31f9f58c908709db7b67e815b2f6c0c6df8540edc4be43752d2","observation_id":"1aef020a-1e84-4591-9cd9-b677e0a411f4","resolution":{"observed_at":"2026-08-15T21:13:46.105554Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.624341Z","title":"1998, ApJ, 508, 859, doi: 10.1086/306426","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.624341Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:df6c3e2aec4792146cc6369b6d3ba924547d61e3776b92f8db87cfd7b64203e0","observation_id":"208d74e1-2f5e-49d2-b598-d64e72421f49","resolution":{"observed_at":"2026-08-15T21:13:44.624341Z","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":"10.1086/507600","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.963774Z","title":null,"venue":null,"work_id":"d9936986-0f23-4699-a8aa-e2573f26d1b8","year":2006},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.629837Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:59e8e6efc73bfc3e8b8c0031294baa5d0c8af0c4641219e3c6d157d59adf53df","observation_id":"5518c969-b5c4-46af-8a43-19043a0850db","resolution":{"observed_at":"2026-08-15T21:13:46.013723Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.686772Z","title":"2015, ApJ, 805, 105, doi: 10.1088/0004-637X/805/2/105","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.686772Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:f1d8d86d4c80079a4ade25129fde78529977d0af2356ff38e0fbd943787d5734","observation_id":"4adf8b47-2b56-4fb3-b1e8-aa25ee474cc9","resolution":{"observed_at":"2026-08-15T21:13:44.686772Z","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":"2026-08-15T21:13:44.718299Z","title":"W., & Tchekhovskoy, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.718299Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:968f7f33d7c5f6e50c34c987e73053f561863b60892b5c837a140d01ed862b61","observation_id":"d4bd7278-dffb-4aed-b8b3-dfb23dbe37d6","resolution":{"observed_at":"2026-08-15T21:13:44.718299Z","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":"2026-08-15T21:13:44.749802Z","title":"2011, ApJ, 741, 93, doi: 10.1088/0004-637X/741/2/93 Falceta-Gonc ¸alves, D., & Kowal, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.749802Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:64f35eb9cbea21b1f8b0a7ce959cc374f6d93bd0232d5ef0e82a033f8dbc4ea8","observation_id":"728b156e-b22d-4639-ad1b-cb8232975de3","resolution":{"observed_at":"2026-08-15T21:13:44.749802Z","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":"2026-08-15T21:13:44.754909Z","title":"2011, NewAR, 55, 166, doi: 10.1016/j.newar.2011.08.002","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.754909Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:9b15bac7da9e2386a79f048b5dc0b12f80d734570459e87961b4cde0a7e2754b","observation_id":"cea315f7-52a8-4623-a0c7-e1e04c2c3321","resolution":{"observed_at":"2026-08-15T21:13:44.754909Z","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":"2026-08-15T21:13:44.759640Z","title":"F., Gammie, C","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.759640Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:603b772180690e1555d5eda1a8f78c882d59235f9bd5df4c0ba629787da4ad16","observation_id":"ac0f2f90-7f8e-487a-9d25-1d0a8c06d430","resolution":{"observed_at":"2026-08-15T21:13:44.759640Z","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":"2026-08-15T21:13:44.764653Z","title":"M., & Davis, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.764653Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:f06901567bd993a5cbdad89b95e325125cab398e74b86111208368abf8eccff4","observation_id":"6e18402b-aa7c-4d90-8299-d4b22bfa76a0","resolution":{"observed_at":"2026-08-15T21:13:44.764653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.05241","last_updated":"2019-03-12T22:22:10Z","snapshot_observed_at":"2026-08-14T17:03:12.540375Z","submitted_at":"2019-03-12T22:22:10Z","title":"Probing the Physical Properties of the Corona in Accreting Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.05241","snapshot_observed_at":"2026-08-15T21:13:44.768876Z","title":"2019, BAAS, 51, 126, doi: 10.48550/arXiv.1903.05241","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.768876Z"},"links":{"cited_paper":"/paper/1903.05241","citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:76fe4bb80d9b7e00b4e1b4093b1e0ee11e4c4a110d08dbb4c0c66c197ffc93e6","observation_id":"1228ed3c-8951-4b7e-90fa-a42411b74586","resolution":{"observed_at":"2026-08-15T21:13:44.768876Z","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":"2026-08-15T21:13:46.960081Z","title":"2020, Fundamentals of Astrophysical Fluid Dynamics (Springer)","venue":null,"work_id":"c2643421-e47a-400f-be09-53690e677358","year":2020},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.773776Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:5cb6a71501bb7598c074eac1f272707c1f9f18bdc7fe962bf6e3502d7657a082","observation_id":"db19cb11-aab2-40f3-9074-94c16b08e80b","resolution":{"observed_at":"2026-08-15T21:13:47.048348Z","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":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.778625Z","title":"2008, Black-Hole Accretion Disks — Towards a New Paradigm —","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.778625Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:0194400ddcf25e92778c9c1eea8af921c6157c6fb809a4b4fbd58c96d6edd246","observation_id":"61b4588f-56d8-490c-8f4e-273280b5285d","resolution":{"observed_at":"2026-08-15T21:13:44.778625Z","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":"2026-08-15T21:13:44.828211Z","title":"2021, NewAR, 92, 101610, doi: 10.1016/j.newar.2021.101610","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.828211Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:69e193898745582e86a7943ea82ca0e06000d33135ed0a8602914f4b18df489e","observation_id":"9aa06b0d-9671-4532-8945-6d0fa49e4517","resolution":{"observed_at":"2026-08-15T21:13:44.828211Z","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":"2026-08-15T21:13:44.867747Z","title":"E., & Contopoulos, I","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.867747Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:e7f46213ff4f7c250414cadf42745b43fc0beebe590c6e83506e282331933bd9","observation_id":"9e7aad00-4c99-412b-9266-4f8ff287d3b5","resolution":{"observed_at":"2026-08-15T21:13:44.867747Z","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":"2026-08-15T21:13:44.922639Z","title":"2022, Science, 378, 650, doi: 10.1126/science.add5399","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.922639Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:b03787deb1d198ba1583be8a324f4c2088a4e8464c5528a897575d6c094e93f7","observation_id":"5346958b-8399-40c5-bade-7da4aa769e05","resolution":{"observed_at":"2026-08-15T21:13:44.922639Z","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":"10.1063/1.1537911","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.832689Z","title":null,"venue":null,"work_id":"5a99548d-520d-493a-a478-edb47476baa7","year":2002},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.927519Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:e337aebafc02cb8ca606726099eb75dd03db8fa791cdd799ffc1b9e91ea81356","observation_id":"d2f98d40-5d37-4fc9-8229-e2d55135d5e4","resolution":{"observed_at":"2026-08-15T21:13:45.876101Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.931935Z","title":"M., Cen, R., Ostriker, J","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.931935Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:a984630ef6ba0c897c32382683a33d3a1c99b9f8a97813e3a9e0c7465b3f5ea9","observation_id":"b7424693-d56f-4fe9-a025-65f8878d141a","resolution":{"observed_at":"2026-08-15T21:13:44.931935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20053372","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.727525Z","title":null,"venue":null,"work_id":"e9d4232e-500e-4cae-82ea-707f33a2fbc0","year":2005},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.936032Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:e9e29947ba3d130f03cb8d271657edef997925e14e78dc54f1d86ee920f66dd2","observation_id":"b29d5c56-8270-441a-b254-ed9f2ce0b43a","resolution":{"observed_at":"2026-08-15T21:13:45.751631Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.941148Z","title":"2003, PhRvD, 67, 043505, doi: 10.1103/PhysRevD.67.043505","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.941148Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:969bd20573d1b850d942a2bef536ce78d17d15dec183dfa9597447129feb746e","observation_id":"3b37d76d-967e-444f-b5a6-bba78813718c","resolution":{"observed_at":"2026-08-15T21:13:44.941148Z","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":"2026-08-15T21:13:46.810408Z","title":null,"venue":null,"work_id":"fed193af-3bca-4851-84fe-3464ec201d1f","year":2021},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.946596Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:bbb43b06902f3b39fc279fc21c80012aabd69f9b89d782b20a3186e9cb3aa789","observation_id":"99620085-f190-43ed-ba52-ad6d847f8c47","resolution":{"observed_at":"2026-08-15T21:13:46.869670Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:13:44.950976Z","title":"C., & Narayan, R","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.950976Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:1e6ea76bc017c4d03f26c9057d8cffc91acd267d78397a64cac1111a55c47790","observation_id":"48ac710a-3148-485f-9c08-c263d53744de","resolution":{"observed_at":"2026-08-15T21:13:44.950976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201117369","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.707038Z","title":"2012, A&A, 537, A18, doi: 10.1051/0004-6361/201117369","venue":null,"work_id":"18054803-19f2-4567-aaa2-8d83ce3e52b0","year":2012},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.955193Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:3580a616074d141b2a6a852a5d48cf7747ceb26e40716da97c6e5a0e3f75c05e","observation_id":"3f35a309-96cf-49b3-9c46-7e196e723c65","resolution":{"observed_at":"2026-08-15T21:13:45.710928Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:44.959518Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.959518Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:24a1585e7bdacf9879cff366b8872f01b103cc11db59ac4265ecd15e20184d42","observation_id":"e48d45b4-8e7a-48a3-bb11-8762ec9435cb","resolution":{"observed_at":"2026-08-15T21:13:44.959518Z","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":"2026-08-15T21:13:46.797762Z","title":null,"venue":null,"work_id":"0b650c6b-4c17-43ac-b85a-635e27f21d58","year":1978},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:44.963643Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:62ef01f72b27f187a1208c338018e36664e61e357452a4c40c705bbb2bb801fd","observation_id":"e9c74c9c-6f20-49d2-9a88-23fa3b44e216","resolution":{"observed_at":"2026-08-15T21:13:46.801955Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:13:45.005640Z","title":"2022, MNRAS, 511, 3795, doi: 10.1093/mnras/stac285 O’Dell, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.005640Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:44bea798f592030487882ee85e431cfd75f745cd5e5c55c0cbcffce7f2d36aef","observation_id":"7f4c612d-2b91-4bff-9b55-186e051bbefd","resolution":{"observed_at":"2026-08-15T21:13:45.005640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa3920","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.685799Z","title":"K., & Chattopadhyay, I","venue":null,"work_id":"05c23806-cff1-412a-8f38-98cda1a71e48","year":2021},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.042463Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:621524047702525e91ab8683f19769ba469b9987fce2d0173a7f05743b144a2c","observation_id":"14a83d6f-ede2-47fe-8d51-b0188ac6ceda","resolution":{"observed_at":"2026-08-15T21:13:45.689966Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.078286Z","title":"C., & Miller, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.078286Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:5dfb070bc3fa9ad14cebbe4b8b78360af620b602a2b4be2ec7aafd6ce08ccf68","observation_id":"71ecc328-d6c3-4a6e-bb13-8986c9c16f3b","resolution":{"observed_at":"2026-08-15T21:13:45.078286Z","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":"2026-08-15T21:13:45.099235Z","title":"K., M´endez, M., & Garc´ıa, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.099235Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:a5705fd53fc349e22fe5303fc31c3c31b300875d81d12a0d03e8e070acec1eab","observation_id":"5f35848c-4cf7-4609-94ac-8e65ec1f4ead","resolution":{"observed_at":"2026-08-15T21:13:45.099235Z","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":"2026-08-15T21:13:45.103990Z","title":"A., Sokolov, D","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.103990Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:8d3e72204db80685071b73de2b160394ec2585d71c4c6e2eb2109aefac267216","observation_id":"b66ee2cd-762d-4569-80f9-dba06f4b487e","resolution":{"observed_at":"2026-08-15T21:13:45.103990Z","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":"2026-08-15T21:13:45.108866Z","title":"B., & Lightman, A","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.108866Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:da6c24b17f130e77f33c3020be52882119cef4fc5417bb38dc51af474a8a87be","observation_id":"7a8dcc82-975a-444d-98a8-ce763b7dcc5b","resolution":{"observed_at":"2026-08-15T21:13:45.108866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0741-3335/47/5a/015","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.648221Z","title":"2005, Plasma Physics and Controlled Fusion, 47, A205, doi: 10.1088/0741-3335/47/5A/015","venue":null,"work_id":"3fe4ce62-ec36-476c-be23-a3e8a8c76983","year":2005},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.112841Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:cf687528cf942d9b515b685c20e2a4322bb0da1ed105bb3fcacbee209aba2e50","observation_id":"c92babaa-77f7-4964-b80d-b29c12693045","resolution":{"observed_at":"2026-08-15T21:13:45.653506Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.117003Z","title":"I., & Sunyaev, R","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.117003Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:53c0515349e8128943f519a87b5ce87ab4dfd232f830e3e848052f28de9e682b","observation_id":"c1b504ab-b293-47e6-8594-dc904572d114","resolution":{"observed_at":"2026-08-15T21:13:45.117003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/782/2/108","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.634915Z","title":"2014, ApJ, 782, 108, doi: 10.1088/0004-637X/782/2/108","venue":null,"work_id":"9a8c2015-463b-4b35-b8b2-651474abf677","year":2014},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.122061Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:92ec31273f29867c2b163123efb86a5ffaf6c6a8ca61e32406f4d773c432426e","observation_id":"db883cdb-6f87-4cdd-a0fd-74207b2b8baf","resolution":{"observed_at":"2026-08-15T21:13:45.638816Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.127249Z","title":"2025, MNRAS, 536, 3284, doi: 10.1093/mnras/stae2514","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.127249Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:256147751e30431c36c006ec27aca801c542c21a04e43427b5f92f3f9a2dc0b8","observation_id":"f9d903c2-8e90-4e93-a30d-3813dd8ac9ee","resolution":{"observed_at":"2026-08-15T21:13:45.127249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/sty2917","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.475894Z","title":"K., & Chattopadhyay, I","venue":null,"work_id":"c3ef1062-4b8c-4f80-958f-2722cd539b8e","year":2019},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.147298Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:0472114a1879f7c39cf69fd182a480333c603396f63b2899eddb1f22f95a61c5","observation_id":"67c1850b-e955-4b61-bf8e-df2ab66d8541","resolution":{"observed_at":"2026-08-15T21:13:45.540418Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.239295Z","title":null,"venue":null,"work_id":null,"year":1959},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.239295Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:6f55b9907e25eecd5a87bf8bc2e9fb7f67037c4d09f7d7e02fbb2c523297595d","observation_id":"9a40f1d5-9abd-4ffa-b398-40974f3c3549","resolution":{"observed_at":"2026-08-15T21:13:45.239295Z","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":"2026-08-15T21:13:46.768434Z","title":"C., Ramsey, B., O’Dell, S., et al","venue":null,"work_id":"5f075784-e3cb-47c5-b6f2-7931f136c08b","year":2016},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.294868Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:853686a7ada788144456668d01cd93e9e74b5c1ba36b213465ea36830304808e","observation_id":"8c531086-9605-4e7f-89e7-a47fff44dc36","resolution":{"observed_at":"2026-08-15T21:13:46.772463Z","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":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.356104Z","title":"9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, ed","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.356104Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:545fba84e4bdcf7e7871e9f9b40608375412a748fc6096d690c929b770edba02","observation_id":"7dbd331b-5639-4905-92d8-46239184f836","resolution":{"observed_at":"2026-08-15T21:13:45.356104Z","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":"2026-08-15T21:13:45.392255Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.392255Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:0238f9e46fff1cc93eaad8ac7aec05e809a5d74dbe5c4059f076dfc2f3a43f4f","observation_id":"8d2dd7fd-34f4-4bf1-a0c9-c7d12b7cfa55","resolution":{"observed_at":"2026-08-15T21:13:45.392255Z","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":"2026-08-15T21:13:45.397426Z","title":"N., Du, Y ., Prather, B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.397426Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:2cf694f4a63fa4606a91bb342e126a7a53c9b3331c178bc3e77f3cb0e515ad0e","observation_id":"74198522-8a38-4edd-80bd-506d043f1528","resolution":{"observed_at":"2026-08-15T21:13:45.397426Z","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":"2026-08-15T21:13:46.557252Z","title":"2019, Science China","venue":null,"work_id":"b0c6e708-c5d2-4b3c-b2ab-eade97155198","year":2019},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.401948Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:48a8ef2d81e046403e2c821f83d2c4ca6971bd600665d52307c088a163df53f5","observation_id":"bff29b13-7676-45c0-bf33-ba351d8d44a9","resolution":{"observed_at":"2026-08-15T21:13:46.664368Z","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":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:13:45.405677Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T21:13:45.405677Z"},"links":{"citing_paper":"/paper/2505.10460"},"observation_digest":"sha256:4939024849addbb3c36f8b8ead86acf1a83b57ebc570bf0a97427da23aac066d","observation_id":"2827e905-6b60-4f7b-92f7-dd133b4d0652","resolution":{"observed_at":"2026-08-15T21:13:45.405677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.10460","last_updated":"2025-05-15T16:16:36Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-15T22:53:22.367931Z","submitted_at":"2025-05-15T16:16:36Z","title":"Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields"},"reference_resolution":{"displayed":48,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":33,"verified_exact":11,"verified_fuzzy":4},"total_outbound_references":48},"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 48 of 48 outbound references and 0 inbound Pith citation observations for arXiv:2505.10460."}