{"as_of":"2026-08-07T16:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7a19390bb3d50b8323526ccf8cec3a2b7b6d269fd46ea570c01dc50e849f60f9","coverage":[{"denominator":2,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T17:53:06.869276Z","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":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T19:06:37.234962Z","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":"2508.15624","last_updated":"2025-08-21T14:50:45Z","snapshot_observed_at":"2026-08-05T23:28:25.148061Z","submitted_at":"2025-08-21T14:50:45Z","title":"Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\\odot}$ neutron star at solar metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.15624","snapshot_observed_at":"2026-08-03T19:06:37.234962Z","title":"& Stevenson, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.02296","last_updated":"2026-06-25T11:52:32Z","snapshot_observed_at":"2026-08-06T16:51:44.805591Z","submitted_at":"2025-12-02T00:25:41Z","title":"Probing the redshift evolution and sub-populations of binary neutron stars with the Einstein Telescope","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-03T19:06:37.234962Z"},"links":{"cited_paper":"/paper/2508.15624","citing_paper":"/paper/2512.02296"},"observation_digest":"sha256:f808a697b012a06a8bcbd180d6231f9a7ab6afa5e39404b4c115134c00552beb","observation_id":"54884522-3178-492d-83ce-a2bf12e2bd89","resolution":{"observed_at":"2026-08-03T19:06:37.234962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2508.15624/citation-record","integrity":"/paper/2508.15624/integrity","json":"/paper/2508.15624/citation-record.json","paper":"/paper/2508.15624"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:53:07.376733Z","title":"P., et al., 2017a, Phys","venue":null,"work_id":"b0064699-7e08-4eec-aca8-b5b6766da88a","year":2020},"citing_paper":{"arxiv_id":"2508.15624","last_updated":"2025-08-21T14:50:45Z","snapshot_observed_at":"2026-08-05T23:28:25.148061Z","submitted_at":"2025-08-21T14:50:45Z","title":"Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\\odot}$ neutron star at solar metallicity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-05T17:53:06.766552Z"},"links":{"citing_paper":"/paper/2508.15624"},"observation_digest":"sha256:045028045256a09839abbfe07ec569bc3ab9c64ca886661094c45c4155c31743","observation_id":"7b2fd76b-3c8a-4d32-ae69-f636e7751a59","resolution":{"observed_at":"2026-08-05T17:53:07.503356Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.01993","last_updated":"2025-07-02T17:47:23Z","snapshot_observed_at":"2026-07-06T20:45:59.818273Z","submitted_at":"2025-03-03T19:10:35Z","title":"The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds","version":2},"cited_work":{"arxiv_id":"2503.01993","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.01993","snapshot_observed_at":"2026-08-05T17:53:07.103867Z","title":"The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds","venue":"astro-ph.SR","work_id":"d4d21ad0-4511-43c3-a388-e10f51f101d8","year":2025},"citing_paper":{"arxiv_id":"2508.15624","last_updated":"2025-08-21T14:50:45Z","snapshot_observed_at":"2026-08-05T23:28:25.148061Z","submitted_at":"2025-08-21T14:50:45Z","title":"Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\\odot}$ neutron star at solar metallicity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-05T17:53:06.869276Z"},"links":{"cited_paper":"/paper/2503.01993","citing_paper":"/paper/2508.15624"},"observation_digest":"sha256:5915df94b3a0e6d7ce9f5efd454b92db8d5e16e317d04f8160288abd4f07e8a5","observation_id":"13dae428-2d7c-4b13-acdd-e28dc5baf86f","resolution":{"observed_at":"2026-08-05T17:53:07.220522Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2508.15624","last_updated":"2025-08-21T14:50:45Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-05T23:28:25.148061Z","submitted_at":"2025-08-21T14:50:45Z","title":"Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\\odot}$ neutron star at solar metallicity"},"reference_resolution":{"displayed":2,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":1,"verified_fuzzy":1},"total_outbound_references":2},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2508.15624."}