{"as_of":"2026-08-20T07:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:497667b873931d4d47d27ec5e64beaaa8f3e0c9e08431259048c60bcba5aaf08","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:41:37.506079Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-07T22:24:11.004806Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-15T21:41:37.506079Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-18T12:04:35.811320Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.506079Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:bfb2ed327dbc9d32581b88c103d3bf26f779325346b0f15ece198d96096f073d","observation_id":"1edbdef0-b426-4522-b9d8-0cd1cc67b912","resolution":{"observed_at":"2026-08-15T21:41:37.506079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-05T17:13:11.758236Z","title":null,"venue":null,"work_id":null,"year":2040},"citing_paper":{"arxiv_id":"2508.16855","last_updated":"2025-08-23T00:57:55Z","snapshot_observed_at":"2026-08-17T22:20:12.507635Z","submitted_at":"2025-08-23T00:57:55Z","title":"$\\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer","version":1},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-08-05T17:13:11.758236Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2508.16855"},"observation_digest":"sha256:284b7a8c75fda40835e008d741d5cf10faa7e87e85567155c64802a181eceec8","observation_id":"0b64b7d4-8f48-4227-96c1-213c971b1513","resolution":{"observed_at":"2026-08-05T17:13:11.758236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":"2111.02439","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-07-07T22:24:11.004806Z","title":"What really makes an accretion disc MAD","venue":"astro-ph.HE","work_id":"cb9d1a42-b7e3-447a-8db6-72c63e95edb9","year":2021},"citing_paper":{"arxiv_id":"2607.05246","last_updated":"2026-08-14T16:16:15Z","snapshot_observed_at":"2026-08-19T23:10:51.130180Z","submitted_at":"2026-07-06T15:55:51Z","title":"The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2607.05246"},"observation_digest":"sha256:d88149ac1813862f2a5947d6d1dcc23042a6800994d54406fe730b53e6cbfb45","observation_id":"a1ee7355-9c87-49c7-ac82-f1237833f607","resolution":{"observed_at":"2026-07-07T22:24:11.006043Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-01T13:29:31.626208Z","title":"arXiv:2111.02439 [astro-ph] , author =","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19113","last_updated":"2026-07-21T13:56:38Z","snapshot_observed_at":"2026-08-18T11:59:07.495880Z","submitted_at":"2026-07-21T13:56:38Z","title":"Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-01T13:29:31.626208Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2607.19113"},"observation_digest":"sha256:b1013aff64b05cf7d758630871948f626d0cafd59c647306e0f0a8504f0f8a9f","observation_id":"f6f0d0b3-84c7-4070-ac14-ec01bbfad43f","resolution":{"observed_at":"2026-08-01T13:29:31.626208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-15T15:15:05.055393Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.01249","last_updated":"2026-08-02T14:01:09Z","snapshot_observed_at":"2026-08-17T22:17:33.013731Z","submitted_at":"2026-08-02T14:01:09Z","title":"The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504","version":1},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-08-15T15:15:05.055393Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2608.01249"},"observation_digest":"sha256:a1b18aab813117817461ecbc451dd18ae276aca097b2081938b26fc2e692dc36","observation_id":"e3ce9a07-b812-40b9-bee7-d0047ede3333","resolution":{"observed_at":"2026-08-15T15:15:05.055393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-06T00:18:32.657365Z","title":null,"venue":null,"work_id":null,"year":2040},"citing_paper":{"arxiv_id":"2608.01413","last_updated":"2026-08-02T17:48:09Z","snapshot_observed_at":"2026-08-17T17:07:13.294766Z","submitted_at":"2026-08-02T17:48:09Z","title":"Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T00:18:32.657365Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2608.01413"},"observation_digest":"sha256:29c8811e2e83a1fecf2d2ed260f5150a217f90babd9662d821191446d8ce732c","observation_id":"5c3d9b5a-095e-4fc3-a6bf-16e58aa6d2c1","resolution":{"observed_at":"2026-08-06T00:18:32.657365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2111.02439/citation-record","integrity":"/paper/2111.02439/integrity","json":"/paper/2111.02439/citation-record.json","paper":"/paper/2111.02439"},"outbound":[],"paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T17:44:13.601485Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2111.02439."}