{"as_of":"2026-08-12T03:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ad59e84d70ea1c8ac3767610362bec265944532e4fa52d9e085b46605f0e21c9","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:56:11.336337Z","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":"2026-05-18T03:40:50.849293Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.17408","last_updated":"2024-05-27T17:56:05Z","snapshot_observed_at":"2026-08-02T17:18:42.121438Z","submitted_at":"2024-05-27T17:56:05Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.17408","snapshot_observed_at":"2026-08-11T22:56:11.336337Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03010","last_updated":"2024-12-04T04:01:09Z","snapshot_observed_at":"2026-08-11T22:49:31.886224Z","submitted_at":"2024-12-04T04:01:09Z","title":"Energy extraction from a rotating black hole via magnetic reconnection: parameters in reconnection models","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T22:56:11.336337Z"},"links":{"cited_paper":"/paper/2405.17408","citing_paper":"/paper/2412.03010"},"observation_digest":"sha256:f0aae0d6271ded31ca2481095f9b924b01562223ce80b727bc64b57973d1d130","observation_id":"f8e3d806-1da0-4bcf-a68a-773d4cf8c3fa","resolution":{"observed_at":"2026-08-11T22:56:11.336337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.17408","last_updated":"2024-05-27T17:56:05Z","snapshot_observed_at":"2026-08-02T17:18:42.121438Z","submitted_at":"2024-05-27T17:56:05Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.17408","snapshot_observed_at":"2026-08-11T04:37:46.410520Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.04019","last_updated":"2024-12-25T02:25:55Z","snapshot_observed_at":"2026-08-11T18:09:07.991010Z","submitted_at":"2024-12-25T02:25:55Z","title":"Generally relativistic description of fast magnetic reconnection induced by thermal electromotive force","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T04:37:46.410520Z"},"links":{"cited_paper":"/paper/2405.17408","citing_paper":"/paper/2501.04019"},"observation_digest":"sha256:f3b59848b6f34ddb869a1c1bb6b0eaf2ea6c1423b785e061a4d24c239e0a906e","observation_id":"a50d8c19-4bac-4c0d-966b-50f523210b0d","resolution":{"observed_at":"2026-08-11T04:37:46.410520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.17408","last_updated":"2024-05-27T17:56:05Z","snapshot_observed_at":"2026-08-02T17:18:42.121438Z","submitted_at":"2024-05-27T17:56:05Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","version":1},"cited_work":{"arxiv_id":"2405.17408","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.17408","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","venue":null,"work_id":"1e26dacb-7b0d-45bc-8106-ab7be0ef0926","year":2024},"citing_paper":{"arxiv_id":"2510.23292","last_updated":"2026-05-10T04:06:46Z","snapshot_observed_at":"2026-08-11T16:14:20.155001Z","submitted_at":"2025-10-27T13:01:09Z","title":"Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-18T03:37:40.315677Z"},"links":{"cited_paper":"/paper/2405.17408","citing_paper":"/paper/2510.23292"},"observation_digest":"sha256:bfad8e38de18a0c9ad20ff767f59105a790ce4ff50a2237804c6be54bd779db0","observation_id":"7b8587b3-becd-43c2-87e4-d5f80883ccec","resolution":{"observed_at":"2026-05-18T03:40:50.852728Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.17408","last_updated":"2024-05-27T17:56:05Z","snapshot_observed_at":"2026-08-02T17:18:42.121438Z","submitted_at":"2024-05-27T17:56:05Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","version":1},"cited_work":{"arxiv_id":"2405.17408","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.17408","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion","venue":null,"work_id":"1e26dacb-7b0d-45bc-8106-ab7be0ef0926","year":2024},"citing_paper":{"arxiv_id":"2605.08597","last_updated":"2026-05-09T01:35:35Z","snapshot_observed_at":"2026-07-06T23:20:47.880233Z","submitted_at":"2026-05-09T01:35:35Z","title":"General Grad-Shafranov Equation","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-12T01:23:25.135358Z"},"links":{"cited_paper":"/paper/2405.17408","citing_paper":"/paper/2605.08597"},"observation_digest":"sha256:872097554b53f1d67db62b561faa982a438797dcfeccfd269facb9cee25b9152","observation_id":"f8b48e48-8ef6-4881-8d1f-92987c7254c4","resolution":{"observed_at":"2026-05-12T08:01:29.905223Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2405.17408/citation-record","integrity":"/paper/2405.17408/integrity","json":"/paper/2405.17408/citation-record.json","paper":"/paper/2405.17408"},"outbound":[],"paper":{"arxiv_id":"2405.17408","last_updated":"2024-05-27T17:56:05Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-02T17:18:42.121438Z","submitted_at":"2024-05-27T17:56:05Z","title":"Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2405.17408."}