{"as_of":"2026-08-22T10:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:59a4bb52a53aaef8208a64d25ddd6286e5f360804c1fca1b485fece776a2ec6c","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":"2026-08-22T06:32:14.747728+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":"2026-08-04T18:26:36.462946Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.01205","last_updated":"2020-08-25T12:58:08Z","snapshot_observed_at":"2026-08-05T14:06:08.406079Z","submitted_at":"2020-04-02T18:05:13Z","title":"The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.01205","snapshot_observed_at":"2026-08-04T18:26:36.462946Z","title":", author Fragos , T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.10002","last_updated":"2025-09-12T06:54:44Z","snapshot_observed_at":"2026-08-08T22:32:29.861055Z","submitted_at":"2025-09-12T06:54:44Z","title":"High Power Accretion in Massive Binary Systems and the Impact of Metallicity","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-04T18:26:36.462946Z"},"links":{"cited_paper":"/paper/2004.01205","citing_paper":"/paper/2509.10002"},"observation_digest":"sha256:26ba3880517cb2461463594b670e4599021885f7b8d5f98d91184d41eead2f9a","observation_id":"0d23f36d-fb3b-4432-abf2-a2055c803f8f","resolution":{"observed_at":"2026-08-04T18:26:36.462946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.01205","last_updated":"2020-08-25T12:58:08Z","snapshot_observed_at":"2026-08-05T14:06:08.406079Z","submitted_at":"2020-04-02T18:05:13Z","title":"The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.01205","snapshot_observed_at":"2026-07-31T05:12:17.050532Z","title":"Misra, T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.24951","last_updated":"2026-07-27T18:02:05Z","snapshot_observed_at":"2026-08-15T20:15:57.499063Z","submitted_at":"2026-07-27T18:02:05Z","title":"Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-31T05:12:17.050532Z"},"links":{"cited_paper":"/paper/2004.01205","citing_paper":"/paper/2607.24951"},"observation_digest":"sha256:1d909eaa1f5ffee803fc2f5740dae68ddac3a66a37f6fd401c220a2a97aed83c","observation_id":"38d1ba54-96ec-4541-b007-0404093a5973","resolution":{"observed_at":"2026-07-31T05:12:17.050532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2004.01205/citation-record","integrity":"/paper/2004.01205/integrity","json":"/paper/2004.01205/citation-record.json","paper":"/paper/2004.01205"},"outbound":[],"paper":{"arxiv_id":"2004.01205","last_updated":"2020-08-25T12:58:08Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-05T14:06:08.406079Z","submitted_at":"2020-04-02T18:05:13Z","title":"The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2004.01205."}