{"as_of":"2026-08-11T06:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:50bfa955d246ddcff58a1e90856933555bb7bc3bcd64779c3e15d00a0da69c5c","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:23:30.652773Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.09556","last_updated":"2025-02-05T13:56:37Z","snapshot_observed_at":"2026-07-06T19:50:29.247307Z","submitted_at":"2024-11-14T16:08:07Z","title":"Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09556","snapshot_observed_at":"2026-08-10T17:23:30.652773Z","title":"arXiv:2411.09556","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12448","last_updated":"2025-02-20T20:58:02Z","snapshot_observed_at":"2026-08-10T17:09:14.765622Z","submitted_at":"2025-01-21T19:00:09Z","title":"Survey of Radiative, Two-Temperature Magnetically Arrested Simulations of the Black Hole M87* I: Turbulent Electron Heating","version":3},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-10T17:23:30.652773Z"},"links":{"cited_paper":"/paper/2411.09556","citing_paper":"/paper/2501.12448"},"observation_digest":"sha256:11ad2ee3f34f9c1cdc511e004d452bea660b71e859812a93df2063461e24fe9c","observation_id":"c9681352-72fe-4cb2-8323-3e1feb7a5841","resolution":{"observed_at":"2026-08-10T17:23:30.652773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09556","last_updated":"2025-02-05T13:56:37Z","snapshot_observed_at":"2026-07-06T19:50:29.247307Z","submitted_at":"2024-11-14T16:08:07Z","title":"Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*","version":3},"cited_work":{"arxiv_id":"2411.09556","doi":"10.48550/arxiv.2411.09556","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09556","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Two-temperature treatments in magnetically arrested disc GRMHD simulations more accurately predict light curves of Sagittarius A*","venue":"arXiv (Cornell University)","work_id":"331a13a8-e223-4b52-bb68-1b96673d8de8","year":2025},"citing_paper":{"arxiv_id":"2605.09326","last_updated":"2026-05-10T04:59:10Z","snapshot_observed_at":"2026-08-07T18:11:57.481519Z","submitted_at":"2026-05-10T04:59:10Z","title":"Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-12T01:56:14.015267Z"},"links":{"cited_paper":"/paper/2411.09556","citing_paper":"/paper/2605.09326"},"observation_digest":"sha256:05abcee90560ec5d2d814bc62a3460e16fbaa27c27b6b61298070ff6e2a75b78","observation_id":"2209be6c-cc39-4b1b-9ff4-fb5edb187158","resolution":{"observed_at":"2026-05-12T02:01:14.871725Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09556","last_updated":"2025-02-05T13:56:37Z","snapshot_observed_at":"2026-07-06T19:50:29.247307Z","submitted_at":"2024-11-14T16:08:07Z","title":"Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*","version":3},"cited_work":{"arxiv_id":"2411.09556","doi":"10.48550/arxiv.2411.09556","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09556","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Two-temperature treatments in magnetically arrested disc GRMHD simulations more accurately predict light curves of Sagittarius A*","venue":"arXiv (Cornell University)","work_id":"331a13a8-e223-4b52-bb68-1b96673d8de8","year":2025},"citing_paper":{"arxiv_id":"2605.15166","last_updated":"2026-05-14T17:55:06Z","snapshot_observed_at":"2026-08-06T08:33:05.969538Z","submitted_at":"2026-05-14T17:55:06Z","title":"Polarization Signatures from GRMHD Simulations of Black Hole Accretion","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-15T03:06:24.087052Z"},"links":{"cited_paper":"/paper/2411.09556","citing_paper":"/paper/2605.15166"},"observation_digest":"sha256:6c64586056692782b73c6a6fbc26c7595ac7c2fea4d119b5c296ecf5cc74aabe","observation_id":"fcc36688-e1df-4e22-aa29-151dd7945eb2","resolution":{"observed_at":"2026-05-15T03:08:59.122564Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.09556/citation-record","integrity":"/paper/2411.09556/integrity","json":"/paper/2411.09556/citation-record.json","paper":"/paper/2411.09556"},"outbound":[],"paper":{"arxiv_id":"2411.09556","last_updated":"2025-02-05T13:56:37Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T19:50:29.247307Z","submitted_at":"2024-11-14T16:08:07Z","title":"Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2411.09556."}