{"as_of":"2026-08-15T20:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:20d6657cf50a7dc4748572cd5dce63721b00701a811ade3ac315f94d1a3a1c0f","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-10T22:25:42.629865Z","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":"2026-07-10T22:27:36.785108Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.11669","last_updated":"2020-05-31T14:40:16Z","snapshot_observed_at":"2026-08-03T21:39:24.326064Z","submitted_at":"2020-04-24T11:42:41Z","title":"Why the mean mass of primordial black hole distribution is close to 10$M_{\\odot}$","version":3},"cited_work":{"arxiv_id":"2004.11669","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.11669","snapshot_observed_at":"2026-07-10T22:27:36.785108Z","title":"Why the mean mass of primordial black hole distribution is close to 10M ⊙","venue":"astro-ph.CO","work_id":"4e014739-308a-4990-8d8a-30e76dd82e09","year":2020},"citing_paper":{"arxiv_id":"2509.21220","last_updated":"2025-10-31T16:27:32Z","snapshot_observed_at":"2026-08-11T20:50:36.071738Z","submitted_at":"2025-09-25T14:27:13Z","title":"Primordial black holes formation in inflationary $F(R)$ models with scalar fields","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-18T13:58:34.507163Z"},"links":{"cited_paper":"/paper/2004.11669","citing_paper":"/paper/2509.21220"},"observation_digest":"sha256:e008ad38af956efda8ecf40c240ba3ac4222da6b99df62217545d693612fa48e","observation_id":"40990f19-0897-4338-a50c-c0b9f307a559","resolution":{"observed_at":"2026-05-18T14:01:27.468340Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.11669","last_updated":"2020-05-31T14:40:16Z","snapshot_observed_at":"2026-08-03T21:39:24.326064Z","submitted_at":"2020-04-24T11:42:41Z","title":"Why the mean mass of primordial black hole distribution is close to 10$M_{\\odot}$","version":3},"cited_work":{"arxiv_id":"2004.11669","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.11669","snapshot_observed_at":"2026-07-10T22:27:36.785108Z","title":"Why the mean mass of primordial black hole distribution is close to 10M ⊙","venue":"astro-ph.CO","work_id":"4e014739-308a-4990-8d8a-30e76dd82e09","year":2020},"citing_paper":{"arxiv_id":"2607.06737","last_updated":"2026-07-07T19:00:31Z","snapshot_observed_at":"2026-08-02T06:29:17.571222Z","submitted_at":"2026-07-07T19:00:31Z","title":"Effect of post-recombination accretion on primordial binary black hole mergers within virialized dark matter halos","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-10T22:25:42.629865Z"},"links":{"cited_paper":"/paper/2004.11669","citing_paper":"/paper/2607.06737"},"observation_digest":"sha256:51b4fa04594c641c67b0bd5ad46e619abd50dc320a3ba4c57d8255dbe5f12a52","observation_id":"aec34f20-180e-442c-9882-4b9e96a6e8ea","resolution":{"observed_at":"2026-07-10T22:27:36.807686Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2004.11669/citation-record","integrity":"/paper/2004.11669/integrity","json":"/paper/2004.11669/citation-record.json","paper":"/paper/2004.11669"},"outbound":[],"paper":{"arxiv_id":"2004.11669","last_updated":"2020-05-31T14:40:16Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-03T21:39:24.326064Z","submitted_at":"2020-04-24T11:42:41Z","title":"Why the mean mass of primordial black hole distribution is close to 10$M_{\\odot}$"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2004.11669."}