{"as_of":"2026-08-08T10:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e09d7691fbedf3ae8546b2746ded2c190b2d7c74f79607e6075860f53f9f9284","coverage":[{"denominator":49,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":49,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T11:49:30.271081Z","state":"measured"},{"denominator":49,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":49,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+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/2607.19815/citation-record","integrity":"/paper/2607.19815/integrity","json":"/paper/2607.19815/citation-record.json","paper":"/paper/2607.19815"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T11:49:22.494653Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:22.494653Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:90740941286593a285a3a4625ff3fbe0e5096654b08bdf22c005ccb1fcf41cb2","observation_id":"7af71e3c-f34b-42ed-b20c-4e05b161867c","resolution":{"observed_at":"2026-08-01T11:49:22.494653Z","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":"2026-08-01T11:49:22.709246Z","title":"Bondi, On Spherically Symmetrical Accretion, Mon","venue":null,"work_id":null,"year":1952},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:22.709246Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:cb92a3a44e05abd47f8f560b55580cbe2c6dd58eafb704a0e9031e199d64a100","observation_id":"1cfeebb5-a72b-454f-8da5-445bcf766929","resolution":{"observed_at":"2026-08-01T11:49:22.709246Z","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":"2026-08-01T11:49:22.933644Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:22.933644Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:f9f9a1cae7305528ba5f8c45f6dcb91efc277de1151dfcf8c2c5c04434e09213","observation_id":"97a44bf0-56a7-487e-85e1-9b8b80f98b13","resolution":{"observed_at":"2026-08-01T11:49:22.933644Z","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":"2026-08-01T11:49:23.096112Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.096112Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:79e21dce22d73baed282bc66b4ca5e13ece143f7105a9467942b730d7393c5e0","observation_id":"4b53d496-cdc8-4d05-b784-3c4737e04029","resolution":{"observed_at":"2026-08-01T11:49:23.096112Z","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":"2026-08-01T11:49:23.344753Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.344753Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:8043c3159a4456cc58e82014f0c4c6525f8895907e38834d5de3649a21aba62e","observation_id":"52d3cbd9-7ad0-4d46-8d5a-4bb268c198cc","resolution":{"observed_at":"2026-08-01T11:49:23.344753Z","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":"2026-08-01T11:49:23.500384Z","title":null,"venue":null,"work_id":null,"year":1934},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.500384Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:fcd104c3a9f10caba34030cc8a4d556ad0983364902466b3162667575e7d43cd","observation_id":"c2fbd75b-beb9-4178-9987-5db99990b905","resolution":{"observed_at":"2026-08-01T11:49:23.500384Z","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":"2026-08-01T11:49:23.724498Z","title":"Ehlers, General relativity and kinetic theory, inGeneral Relativity and Cosmology, edited by R","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.724498Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:0c17b5051c64085f1ebbc103df4d78da17cd1baedd97c198555d575861305306","observation_id":"fd4230a0-b6e0-4021-96a4-b662a81add8c","resolution":{"observed_at":"2026-08-01T11:49:23.724498Z","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":"2026-08-01T11:49:23.883862Z","title":"Sarbach and T","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.883862Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:7f7c9e3f68fb99f32ee24d96b33f911384018da482ecb5f8a76598a74af213a0","observation_id":"94f7d3f8-ed45-4e1e-80ab-3d458716ea95","resolution":{"observed_at":"2026-08-01T11:49:23.883862Z","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":"2026-08-01T11:49:23.997100Z","title":"Sarbach and T","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:23.997100Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:8c25dc431700ecfd5a343ad5b2e755f1091700befdd72049f965878b2da3022f","observation_id":"48dbbe43-bea8-4215-89b8-08daf3def092","resolution":{"observed_at":"2026-08-01T11:49:23.997100Z","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":"2026-08-01T11:49:24.216794Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:24.216794Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:e7aa1aa9edef8022ca54a9a859d28c6eb3a2f2983ad1176801cd0d370e153745","observation_id":"4b3d52de-c9f1-4aec-aef4-860548e9341d","resolution":{"observed_at":"2026-08-01T11:49:24.216794Z","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":"2026-08-01T11:49:24.390685Z","title":"Andr´ easson, The Einstein–Vlasov system/kinetic theory, Living Rev","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:24.390685Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:ff4f0a0f831f216044f658687ac661ae1ca69a7cfa048d859a4575efd6f915a4","observation_id":"dc63d8b9-fde8-4e93-9a95-c5d32996affa","resolution":{"observed_at":"2026-08-01T11:49:24.390685Z","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":"2026-08-01T11:49:24.586981Z","title":"Rioseco and O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:24.586981Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:7da3dc257756f3554dc50d33ec6ad819caa5af131372bdbfb6a6b35817346d76","observation_id":"e3e23bc0-bad6-47e1-8961-d763d46321ee","resolution":{"observed_at":"2026-08-01T11:49:24.586981Z","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":"2026-08-01T11:49:24.759362Z","title":"Rioseco and O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:24.759362Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:55acd880a87ab2353a74e7b8cc716a9b42cf64d7b82c1a4d6172ccd8fdd05310","observation_id":"de489c81-13ea-4c6a-8c54-29beff79f86c","resolution":{"observed_at":"2026-08-01T11:49:24.759362Z","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":"2026-08-01T11:49:24.913580Z","title":"Cie´ slik and P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:24.913580Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:bf150eabcefa4a19a39503224065f036fbb0a9cf2551fc0b899c76cc96ee542c","observation_id":"ca62cf6a-79ad-4e22-bb82-4e1d7189578f","resolution":{"observed_at":"2026-08-01T11:49:24.913580Z","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":"2026-08-01T11:49:25.030211Z","title":"Cie´ slik, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.030211Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:cfa81d9b5a0f6d08ee50610a2cb7bf2e56d501839427f6ff364f7f09b0dedf35","observation_id":"cd6ed443-4ac2-483b-853d-492832a00f11","resolution":{"observed_at":"2026-08-01T11:49:25.030211Z","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":"2026-08-01T11:49:25.154431Z","title":"Mach and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.154431Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b486964164e64430afac1d36b7f653f17874b07c464c51a6f69e0d894995b083","observation_id":"9d3c804c-e3bf-464c-9de3-a18c1ef50212","resolution":{"observed_at":"2026-08-01T11:49:25.154431Z","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":"2026-08-01T11:49:25.350879Z","title":"Mach and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.350879Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:95cedd478211ee616afc2bc6cd10797589b7c9137e28b769ccdcbfe0d5d2cdbc","observation_id":"8a19c339-2268-45d7-aadb-17d881e07262","resolution":{"observed_at":"2026-08-01T11:49:25.350879Z","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":"2026-08-01T11:49:25.522646Z","title":"Mach and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.522646Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:a3519031ce4b754160fa0d09f3c97f98ae2fd2109ef834b3b68f1102cfb24841","observation_id":"f692a294-b037-49a0-9e4a-0d222a3c943b","resolution":{"observed_at":"2026-08-01T11:49:25.522646Z","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":"2026-08-01T11:49:25.638968Z","title":"Cie´ slik and P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.638968Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:22f46205b10877730cc711030ee44b438f0b782e3a59e641612c99995156ba41","observation_id":"b892b54c-1fb0-442c-a9af-f8d8baf251d6","resolution":{"observed_at":"2026-08-01T11:49:25.638968Z","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":"2026-08-01T11:49:25.681288Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.681288Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b0457872b5784db7ec915b71dfc2b5e7a71b3d699e8c48a64d310a99c2adc757","observation_id":"5f040e32-b114-4787-a824-cab778452534","resolution":{"observed_at":"2026-08-01T11:49:25.681288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.25425","last_updated":"2026-06-25T01:43:52Z","snapshot_observed_at":"2026-08-08T05:57:49.179736Z","submitted_at":"2026-06-24T05:32:56Z","title":"Accretion of a Plasma Vlasov Gas onto a Reissner-Nordstr\\\"om Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.25425","snapshot_observed_at":"2026-08-01T11:49:25.839072Z","title":"Liu and H","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.839072Z"},"links":{"cited_paper":"/paper/2606.25425","citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:2f23749e40a8babb81be8b9e14aa76ded91c140e7ff59e133b8d2b8078c47375","observation_id":"8c3281ec-6455-42b5-8349-4bdefe79f848","resolution":{"observed_at":"2026-08-01T11:49:25.839072Z","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":"2026-08-01T11:49:25.927880Z","title":"Gamboa, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:25.927880Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:8a5641c6801d2589286c3d2c8812e683c26fb29ab443c805ba8d017a98fb84db","observation_id":"355c31b5-5ac8-46ad-b941-d375f7b1106d","resolution":{"observed_at":"2026-08-01T11:49:25.927880Z","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":"2026-08-01T11:49:26.049700Z","title":"Liao and D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.049700Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:06918071c1ccbc6a21c31ded91e0cc7031a1a0754335c91b4e8d91ac8cdf0d8f","observation_id":"cd0d122c-dfc9-46ff-a710-81996cedfbbc","resolution":{"observed_at":"2026-08-01T11:49:26.049700Z","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":"2026-08-01T11:49:26.252246Z","title":"Cai and R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.252246Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:4e9b66d8ef4dd0b5d7c1816cb26c63f29fc381601438be947b1b06e9903ffc9c","observation_id":"69adbb34-e50e-463f-980e-843f849d4970","resolution":{"observed_at":"2026-08-01T11:49:26.252246Z","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":"2026-08-01T11:49:26.413698Z","title":"Momennia and O","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.413698Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:13ac7c473d36f3ed0aa2c27a73a48f9e0fabfb768000147768ea3265c87ead43","observation_id":"4a579092-feef-4c2e-b5d8-f6c7490f2b13","resolution":{"observed_at":"2026-08-01T11:49:26.413698Z","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":"2026-08-01T11:49:26.556980Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.556980Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:82043b9de52b7d8af78e8c3b8c67ba337c4e6717e727ea2b35e287d5fc326e02","observation_id":"5d838d25-3dd0-4ebf-bfe2-75fedb4a34ed","resolution":{"observed_at":"2026-08-01T11:49:26.556980Z","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":"2026-08-01T11:49:26.735274Z","title":"Gabarrete and O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.735274Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:c259a97f0577d85e509937b7454f2fc0d48d747e529d78cd7e9f197e37fc1052","observation_id":"cb7ab0d3-c9b0-4a26-a675-0993a54576d4","resolution":{"observed_at":"2026-08-01T11:49:26.735274Z","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":"2026-08-01T11:49:26.901762Z","title":"Gabarrete and O","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:26.901762Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:a2aae91f13a26e5bd4b42c4747c132d1e0be7491197a42543344a7e06cb70681","observation_id":"8b2a28cc-d189-4507-bc44-dd4b884f9714","resolution":{"observed_at":"2026-08-01T11:49:26.901762Z","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":"2026-08-01T11:49:27.072765Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.072765Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:22b94e415d924a2deb5d6d453a2362eb30495131b13d3273d2d98215edb1bc21","observation_id":"4e2f93d7-2f7b-497b-9735-f0a1761331b4","resolution":{"observed_at":"2026-08-01T11:49:27.072765Z","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":"2026-08-01T11:49:27.210335Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.210335Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b4d34dc2e4c5da8164687355c0f088c45986f5a19973c0f8ff69ef03fdee3bd6","observation_id":"17eddda7-8e2e-4150-880b-060e6115a81a","resolution":{"observed_at":"2026-08-01T11:49:27.210335Z","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":"2026-08-01T11:49:27.396907Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.396907Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:8410353be0e210b18677a325cd1f669126041278e33aa2d5b41e584eb55ebc80","observation_id":"2de471f8-2e09-4a24-aac7-2849429825c4","resolution":{"observed_at":"2026-08-01T11:49:27.396907Z","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":"2026-08-01T11:49:27.535740Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.535740Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:16382a5b29a2b6f6204715712b1565105e68b16135dac5a7f7c347896a84a5cd","observation_id":"03e21597-537e-4cc3-9673-ef8829fa496c","resolution":{"observed_at":"2026-08-01T11:49:27.535740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.08341","last_updated":"2026-07-14T05:43:13Z","snapshot_observed_at":"2026-08-07T05:11:01.551208Z","submitted_at":"2025-06-10T01:53:12Z","title":"A discussion on the symmetry of relativistic Vlasov gas and its accretion in Kerr-Newman black hole","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.08341","snapshot_observed_at":"2026-08-01T11:49:27.719922Z","title":"Liu, A discussion on the symmetry of relativistic Vlasov gas and its accretion in Kerr– Newman black hole, arXiv:2506.08341 (2025)","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.719922Z"},"links":{"cited_paper":"/paper/2506.08341","citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:7b321c83da21fb2e176340ae40fd38b509045b28bbe8b27c7714560aa8f235e3","observation_id":"8b68514b-c939-4e4a-a4ab-54a47d6deb5c","resolution":{"observed_at":"2026-08-01T11:49:27.719922Z","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":"2026-08-01T11:49:27.846996Z","title":"Khan and P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:27.846996Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:fc8e10014a5aa767f989085fd0df4b7db529626ba5ba6e29e1f91014fa62ef9d","observation_id":"df846b82-ca5a-41ed-beb9-fd42860a3a6f","resolution":{"observed_at":"2026-08-01T11:49:27.846996Z","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":"2026-08-01T11:49:28.014731Z","title":"Luepker, Y","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.014731Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b9263e1639909d3df196bbcd57fda29fe2b3c6953cb6d3e33851e34c5eccc039","observation_id":"158537f1-195b-4b85-83bc-db9e345ea728","resolution":{"observed_at":"2026-08-01T11:49:28.014731Z","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":"2026-08-01T11:49:28.158302Z","title":"Rioseco and O","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.158302Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:8e2dcd1b5006608a6c5be400214be8db10ff853788b2967f815851fe7bc63a07","observation_id":"92dde493-12c2-4d06-a930-0e7dc044405a","resolution":{"observed_at":"2026-08-01T11:49:28.158302Z","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":"2026-08-01T11:49:28.315698Z","title":"Rioseco and O","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.315698Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:07a3574f7894405ae0a24af5b486af95a7a62fcbd6357b1e396c52dc6130f5ee","observation_id":"4f713660-c45b-4b25-8f50-5d24a6ea7010","resolution":{"observed_at":"2026-08-01T11:49:28.315698Z","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":"2026-08-01T11:49:28.504653Z","title":"Tejeda, P","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.504653Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:58c9ba547e06c0a2d34d4f8b97be2274f0c6f55dc8f626fee32cce1d97709b6e","observation_id":"35202a79-db08-4fe5-940b-46517aad2aaf","resolution":{"observed_at":"2026-08-01T11:49:28.504653Z","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":"2026-08-01T11:49:28.680477Z","title":"Bakun, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.680477Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:4351d65c044939a6de1bfae22cd47b361ddcc461c7e7d0c5246d0ee24db31e70","observation_id":"469695fa-87bc-4a92-896d-918fe1cb8cc8","resolution":{"observed_at":"2026-08-01T11:49:28.680477Z","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":"2026-08-01T11:49:28.847361Z","title":"Aguayo-Ortiz, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:28.847361Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:d7bfe82cff1195264864c4f5feed8baba943de960d4d6cb69b37d856bb3f042c","observation_id":"23a5137f-8284-4089-affa-e59fee5c9af8","resolution":{"observed_at":"2026-08-01T11:49:28.847361Z","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":"2026-08-01T11:49:29.024716Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.024716Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:5f9d058eae74adfa2e62b62a59fa71e701b12b8f581a800bab45feddaae96be6","observation_id":"315753ed-5208-48aa-a574-e3e9e6ea896a","resolution":{"observed_at":"2026-08-01T11:49:29.024716Z","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":"2026-08-01T11:49:29.205339Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.205339Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b3fc7c126727eb17b705b58d55d9d7384cd82dbd476530e37af3508ee86a6d57","observation_id":"de7f5727-5180-4d55-9d2c-a5c2e112f309","resolution":{"observed_at":"2026-08-01T11:49:29.205339Z","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":"2026-08-01T11:49:29.319942Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.319942Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:5807ade8c6b219dc26ab84b28f77340dd07626a441f6bec5952cc6437fc522f7","observation_id":"cb2bbc2d-d667-459f-b26c-dae63cd2830c","resolution":{"observed_at":"2026-08-01T11:49:29.319942Z","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":"2026-08-01T11:49:29.475827Z","title":"Cie´ slik, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.475827Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:f5910e78eefb04e175229e49495f224ee0454f9c137e7d83c97994688d0d7735","observation_id":"255a7dcd-2568-43a0-ae0c-471dc5459cf4","resolution":{"observed_at":"2026-08-01T11:49:29.475827Z","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":"2026-08-01T11:49:29.614914Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.614914Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:cbdee1cb60c3d928f7c4973a61f0632cf3e2553393e227c36697a98f5bba1d26","observation_id":"7b118d8f-09af-432d-adf1-badd14e6cf43","resolution":{"observed_at":"2026-08-01T11:49:29.614914Z","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":"2026-08-01T11:49:29.787647Z","title":"J¨ uttner, Maxwell’s law of speed distribution in the theory of relativity, Annal","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.787647Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:c416bc23c88c94629162453fd60c76050030aa7481373d5f18eff7433af1f496","observation_id":"f1801353-5457-4e4e-a6f0-dfe692660118","resolution":{"observed_at":"2026-08-01T11:49:29.787647Z","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":"2026-08-01T11:49:29.958011Z","title":"J¨ uttner, The dynamics of an inert gas in the theory of relativity, Ann","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:29.958011Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:4138042cf8fbdc050daef8fe660debef33de13f49197f1ff44a552daee72406e","observation_id":"8d4e457c-63d5-45de-b5bf-7a4849a34f41","resolution":{"observed_at":"2026-08-01T11:49:29.958011Z","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":"2026-08-01T11:49:30.122719Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:30.122719Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:38a758b40afa888b298c85c5e6b859e902ea9130e7626d2e0fa29306d72cb9ea","observation_id":"f5615051-2ae0-478a-a8bd-2951f294c09f","resolution":{"observed_at":"2026-08-01T11:49:30.122719Z","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":"2026-08-01T11:49:30.271081Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T11:49:30.271081Z"},"links":{"citing_paper":"/paper/2607.19815"},"observation_digest":"sha256:b9a3e4261a9eee94db6a7ca73fec019c1fde58e48896d23c1bd6c62f84aec4df","observation_id":"b06bd92e-a6ab-4905-9878-13db1f4dfba5","resolution":{"observed_at":"2026-08-01T11:49:30.271081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.19815","last_updated":"2026-07-22T06:48:50Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-01T21:42:09.236270Z","submitted_at":"2026-07-22T06:48:50Z","title":"Coordinate Independence of the Schwarzschild Black Hole Accretion Vlasov Gas Model"},"reference_resolution":{"displayed":49,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":49,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":49},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 49 of 49 outbound references and 0 inbound Pith citation observations for arXiv:2607.19815."}