{"as_of":"2026-08-09T01:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2c240ba992b1ebc1510e6dc0cf946fe674b0cfd4935fe69d3e8c06382b7b20aa","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T15:19:13.915568Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-20T09:23:10.389350Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":"2012.08785","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Brahma, C.-Y","venue":null,"work_id":"9a40fae2-7a03-4996-ad9c-60db60ed4966","year":2021},"citing_paper":{"arxiv_id":"2205.07787","last_updated":"2023-05-26T11:55:37Z","snapshot_observed_at":"2026-07-06T13:10:28.094958Z","submitted_at":"2022-05-16T16:22:56Z","title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","version":3},"reference_index":178,"source":"pdf_text","source_observed_at":"2026-05-16T11:20:24.345127Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2205.07787"},"observation_digest":"sha256:a7c37252c000f1185fd29cf901e785601d7aba2a72ace6c8d945d725d2a770c8","observation_id":"5faf9565-2ec0-469f-8106-f0d5754a238e","resolution":{"observed_at":"2026-05-16T11:20:25.054209Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-07T19:55:20.482277Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.10053","last_updated":"2025-02-14T10:01:22Z","snapshot_observed_at":"2026-08-07T19:33:37.298320Z","submitted_at":"2025-02-14T10:01:22Z","title":"Complex degenerate metrics in general relativity: a covariant extension of the Moore-Penrose algorithm","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T19:55:20.482277Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2502.10053"},"observation_digest":"sha256:18205fe7ba97be275b12f8e77e4e504258521e64fa4d88db576ad82e214d1ebc","observation_id":"73d30676-12db-43b2-b6be-81709be2460d","resolution":{"observed_at":"2026-08-07T19:55:20.482277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-07T11:26:26.252034Z","title":"Brahma, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.02653","last_updated":"2025-06-03T09:06:31Z","snapshot_observed_at":"2026-08-07T15:39:27.466751Z","submitted_at":"2025-06-03T09:06:31Z","title":"Thermodynamics and Shadows of Kerr black holes endowed with a global monopole charge","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-07T11:26:26.252034Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2506.02653"},"observation_digest":"sha256:8492156bbbfdccc84e63f67598ecaaaf8578bfd5a816f4ccc5400d8e828957fa","observation_id":"3f1becc0-57ec-4676-82bf-5e66a0942632","resolution":{"observed_at":"2026-08-07T11:26:26.252034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-06T18:54:13.494435Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.07372","last_updated":"2025-07-10T01:51:00Z","snapshot_observed_at":"2026-08-09T00:18:53.748403Z","submitted_at":"2025-07-10T01:51:00Z","title":"Polymer Black Hole Surrounded by Quintessence","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T18:54:13.494435Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2507.07372"},"observation_digest":"sha256:06fd34b12610295a215158ee18fae447ec19bb639e6255c1117716e6a4cb42f8","observation_id":"0659897c-c93f-4250-a63a-8823d5fcafc1","resolution":{"observed_at":"2026-08-06T18:54:13.494435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-06T18:26:44.545836Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.08431","last_updated":"2025-07-11T09:17:08Z","snapshot_observed_at":"2026-08-08T05:13:34.757442Z","submitted_at":"2025-07-11T09:17:08Z","title":"Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:44.545836Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2507.08431"},"observation_digest":"sha256:ffdfa542a3d8caf054e88f170ef46a58f748f8dac2e543125f9e7829bd56a373","observation_id":"55c06415-c956-44bf-a719-137d16250159","resolution":{"observed_at":"2026-08-06T18:26:44.545836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-04T17:26:52.767976Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.10953","last_updated":"2025-09-13T19:23:49Z","snapshot_observed_at":"2026-08-07T09:34:45.857018Z","submitted_at":"2025-09-13T19:23:49Z","title":"Observable thin accretion disk around a self-dual black hole in loop quantum gravity","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T17:26:52.767976Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2509.10953"},"observation_digest":"sha256:471bc406ec5b713de43f3c06a48ad0dac7091e3c6dc0a5703a02cf7a823b8b91","observation_id":"78767384-84f6-48cc-a8c6-7c334160c2f7","resolution":{"observed_at":"2026-08-04T17:26:52.767976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":"2012.08785","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Brahma, C.-Y","venue":null,"work_id":"9a40fae2-7a03-4996-ad9c-60db60ed4966","year":2021},"citing_paper":{"arxiv_id":"2601.10806","last_updated":"2026-05-01T06:09:01Z","snapshot_observed_at":"2026-07-06T22:41:53.823272Z","submitted_at":"2026-01-15T19:15:58Z","title":"Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-16T13:33:18.133767Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2601.10806"},"observation_digest":"sha256:b453510d96d5789859f294ee79e8cb1d0021c498251b85484bc8af535ac261be","observation_id":"efd33ab4-3066-4c92-b705-793810306db9","resolution":{"observed_at":"2026-05-16T13:37:57.299974Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":"2012.08785","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Brahma, C.-Y","venue":null,"work_id":"9a40fae2-7a03-4996-ad9c-60db60ed4966","year":2021},"citing_paper":{"arxiv_id":"2603.25084","last_updated":"2026-04-23T10:20:59Z","snapshot_observed_at":"2026-07-06T22:50:37.468743Z","submitted_at":"2026-03-26T06:38:36Z","title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-15T00:56:02.789832Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2603.25084"},"observation_digest":"sha256:fcc80233f0f8618d9791fab0470cab2d8d1b66f6270c109bb25aacee531b439c","observation_id":"a2e8a597-cd60-4734-805c-8133c7bdd2bd","resolution":{"observed_at":"2026-05-15T00:58:25.920679Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":"2012.08785","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Brahma, C.-Y","venue":null,"work_id":"9a40fae2-7a03-4996-ad9c-60db60ed4966","year":2021},"citing_paper":{"arxiv_id":"2604.23163","last_updated":"2026-04-25T06:29:33Z","snapshot_observed_at":"2026-07-06T23:09:23.591544Z","submitted_at":"2026-04-25T06:29:33Z","title":"Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-08T07:52:22.777987Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2604.23163"},"observation_digest":"sha256:6557a90f999cb1d5bdfb41db204a64041d0f2b92a0a984ea1b7feadd75ed6113","observation_id":"4fa5eb8b-1f1c-439d-b5d0-6ea57285610a","resolution":{"observed_at":"2026-05-11T20:51:10.576292Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":"2012.08785","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Brahma, C.-Y","venue":null,"work_id":"9a40fae2-7a03-4996-ad9c-60db60ed4966","year":2021},"citing_paper":{"arxiv_id":"2605.18249","last_updated":"2026-05-18T11:50:45Z","snapshot_observed_at":"2026-07-06T23:29:09.538843Z","submitted_at":"2026-05-18T11:50:45Z","title":"Quasinormal modes of a rotating loop quantum black hole","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-20T09:22:46.533112Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2605.18249"},"observation_digest":"sha256:eb9842dda176375dfc7c56920cebed95d5416a4a97e8749bbf1562e369fa0473","observation_id":"9e0712a8-4027-4497-b047-dd83d7e5b3b7","resolution":{"observed_at":"2026-05-20T09:23:10.391065Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-07-30T18:14:20.851797Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.26882","last_updated":"2026-07-29T13:11:46Z","snapshot_observed_at":"2026-08-01T23:37:39.721715Z","submitted_at":"2026-07-29T13:11:46Z","title":"Junction Conditions, Radial Stability, Thermodynamics, Optical Geometry and Appearance of Polymer-Quintessence Thin-Shell Wormholes","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-30T18:14:20.851797Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2607.26882"},"observation_digest":"sha256:09ffe41b790c74b49804953c909e49b0854e37c127a93575d815fb84a56b9714","observation_id":"7075b4d9-58bc-4f15-bc33-1d19d2882030","resolution":{"observed_at":"2026-07-30T18:14:20.851797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08785","snapshot_observed_at":"2026-08-08T15:19:13.915568Z","title":"Brahma, C.-Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.05328","last_updated":"2026-08-05T18:36:58Z","snapshot_observed_at":"2026-08-09T01:10:15.502744Z","submitted_at":"2026-08-05T18:36:58Z","title":"White Dwarf Stellar Structure from Effective Polymer Geometry in Loop Quantum Gravity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T15:19:13.915568Z"},"links":{"cited_paper":"/paper/2012.08785","citing_paper":"/paper/2608.05328"},"observation_digest":"sha256:c7c38a6daadfe5394f2d2083583aac5701014de55273025a4f8ff56351972bcf","observation_id":"0999b85d-a5bc-4540-b3b5-56918bac4ba6","resolution":{"observed_at":"2026-08-08T15:19:13.915568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2012.08785/citation-record","integrity":"/paper/2012.08785/integrity","json":"/paper/2012.08785/citation-record.json","paper":"/paper/2012.08785"},"outbound":[],"paper":{"arxiv_id":"2012.08785","last_updated":"2021-05-06T17:47:11Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T10:24:57.667665Z","submitted_at":"2020-12-16T08:04:31Z","title":"Testing loop quantum gravity from observational consequences of non-singular rotating black holes"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2012.08785."}