{"as_of":"2026-08-11T06:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d4aadf0e69811c3541dbc717ff2231a6dddc18c327a7ea42ce22d1c57e3f24f6","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":"2026-08-10T20:15:42.950740Z","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":6,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.18773","last_updated":"2024-12-13T19:00:04Z","snapshot_observed_at":"2026-07-06T17:37:09.952632Z","submitted_at":"2024-02-29T00:27:45Z","title":"Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.18773","snapshot_observed_at":"2026-08-10T20:15:42.950740Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.09098","last_updated":"2025-01-15T19:30:59Z","snapshot_observed_at":"2026-08-10T20:08:05.199117Z","submitted_at":"2025-01-15T19:30:59Z","title":"Boosting Supermassive Black Hole Growth in the Early Universe by Fuzzy Dark Matter Solitons","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T20:15:42.950740Z"},"links":{"cited_paper":"/paper/2402.18773","citing_paper":"/paper/2501.09098"},"observation_digest":"sha256:54580afcfebbf674e12c4b053eb357e0d55da0a1906ac626c47a7f38f40b2d94","observation_id":"b870b18e-d1b8-4837-a5e2-7afc76b68e15","resolution":{"observed_at":"2026-08-10T20:15:42.950740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.18773","last_updated":"2024-12-13T19:00:04Z","snapshot_observed_at":"2026-07-06T17:37:09.952632Z","submitted_at":"2024-02-29T00:27:45Z","title":"Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe","version":2},"cited_work":{"arxiv_id":"2402.18773","doi":"10.48550/arxiv.2402.18773","metadata_source":"arxiv_reference","pith_arxiv_id":"2402.18773","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"arXiv (Cornell University)","work_id":"fa52e395-b90b-4a76-87bc-57e11848fe92","year":2025},"citing_paper":{"arxiv_id":"2606.12851","last_updated":"2026-06-11T03:32:59Z","snapshot_observed_at":"2026-08-03T01:02:38.745595Z","submitted_at":"2026-06-11T03:32:59Z","title":"Supermassive Black Hole Assembly from Heavy Seeds with Dynamical Friction in the BRAHMA Simulations: Implications for JWST, LISA, and the Local Universe","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-27T06:55:11.433036Z"},"links":{"cited_paper":"/paper/2402.18773","citing_paper":"/paper/2606.12851"},"observation_digest":"sha256:bd670dbab58bc9b3cf5cd3f7b3fb635abac7220d6e929c707530becb74a11edc","observation_id":"9664a5ed-d27e-4cee-9547-5cd254f3f2c2","resolution":{"observed_at":"2026-06-27T07:00:40.206632Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2402.18773","last_updated":"2024-12-13T19:00:04Z","snapshot_observed_at":"2026-07-06T17:37:09.952632Z","submitted_at":"2024-02-29T00:27:45Z","title":"Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe","version":2},"cited_work":{"arxiv_id":"2402.18773","doi":"10.48550/arxiv.2402.18773","metadata_source":"arxiv_reference","pith_arxiv_id":"2402.18773","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"arXiv (Cornell University)","work_id":"fa52e395-b90b-4a76-87bc-57e11848fe92","year":2025},"citing_paper":{"arxiv_id":"2607.00349","last_updated":"2026-07-01T02:44:05Z","snapshot_observed_at":"2026-08-06T09:26:47.144762Z","submitted_at":"2026-07-01T02:44:05Z","title":"Variability in Supermassive Black-Hole Accretion Rates in Fuzzy Dark Matter Cores due to Black-Hole Wandering","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-02T00:32:55.425952Z"},"links":{"cited_paper":"/paper/2402.18773","citing_paper":"/paper/2607.00349"},"observation_digest":"sha256:6d8383914808d5fc28ef59d732f00f152fa48f07c23a2f6037ab07309c9d5922","observation_id":"ba77b1ff-b839-4bbf-8bfc-fbe8e6ca12b1","resolution":{"observed_at":"2026-07-02T00:36:23.774020Z","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/2402.18773/citation-record","integrity":"/paper/2402.18773/integrity","json":"/paper/2402.18773/citation-record.json","paper":"/paper/2402.18773"},"outbound":[],"paper":{"arxiv_id":"2402.18773","last_updated":"2024-12-13T19:00:04Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T17:37:09.952632Z","submitted_at":"2024-02-29T00:27:45Z","title":"Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe"},"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:2402.18773."}