{"as_of":"2026-08-15T04:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bfaf7c75c491ad679949476c78cde84f9719fb36a4a4e1dde1f32e0d7e8b6897","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T05:35:20.974212Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":"2601.03861","doi":"10.48550/arxiv.2601.03861","metadata_source":"pith","pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":"astro-ph.HE","work_id":"e22ac5d2-09e0-4a38-9d3b-9e086986e1bb","year":2026},"citing_paper":{"arxiv_id":"2604.05046","last_updated":"2026-04-16T14:11:13Z","snapshot_observed_at":"2026-08-13T11:33:49.903700Z","submitted_at":"2026-04-06T18:00:48Z","title":"Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates","version":2},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-05-10T19:36:48.497341Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2604.05046"},"observation_digest":"sha256:e001eb85fb374c2ddbb9d6bc89de5d1414b588755915013092da03f429cb0654","observation_id":"c46c2d83-a3e5-450b-bacf-f164dc694c0f","resolution":{"observed_at":"2026-06-24T15:15:17.732011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":"2601.03861","doi":"10.48550/arxiv.2601.03861","metadata_source":"pith","pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":"astro-ph.HE","work_id":"e22ac5d2-09e0-4a38-9d3b-9e086986e1bb","year":2026},"citing_paper":{"arxiv_id":"2604.05059","last_updated":"2026-08-01T11:24:21Z","snapshot_observed_at":"2026-08-12T12:58:26.373871Z","submitted_at":"2026-04-06T18:08:43Z","title":"Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-10T19:09:10.089741Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2604.05059"},"observation_digest":"sha256:5f2c9a8adfd0dea0916246f1526ede9464fab2245443d11c58fdb391dc09ea05","observation_id":"1f7cb60a-809f-4f82-bd63-c67298eb126c","resolution":{"observed_at":"2026-06-24T15:15:17.732011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-04T05:35:20.974212Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2604.05059","last_updated":"2026-08-01T11:24:21Z","snapshot_observed_at":"2026-08-12T12:58:26.373871Z","submitted_at":"2026-04-06T18:08:43Z","title":"Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-04T05:35:20.974212Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2604.05059"},"observation_digest":"sha256:ab6d29d592f0732dbd65091eaf46bbd91f19ecf8f8b930130487d90222ada413","observation_id":"faad2f8b-e28f-4e94-8b71-c0625f841008","resolution":{"observed_at":"2026-08-04T05:35:20.974212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":"2601.03861","doi":"10.48550/arxiv.2601.03861","metadata_source":"pith","pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":"astro-ph.HE","work_id":"e22ac5d2-09e0-4a38-9d3b-9e086986e1bb","year":2026},"citing_paper":{"arxiv_id":"2605.03128","last_updated":"2026-06-10T19:08:48Z","snapshot_observed_at":"2026-08-14T19:55:26.214896Z","submitted_at":"2026-05-04T20:10:59Z","title":"Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-05-08T17:29:32.083922Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2605.03128"},"observation_digest":"sha256:904c87b39897f243898012f6f62eb377d189163f587d51a7c9d93c4ca72907cd","observation_id":"a25eb4a3-b01d-4158-976d-c8151a4af9d2","resolution":{"observed_at":"2026-06-24T15:15:17.732011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":"2601.03861","doi":"10.48550/arxiv.2601.03861","metadata_source":"pith","pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":"astro-ph.HE","work_id":"e22ac5d2-09e0-4a38-9d3b-9e086986e1bb","year":2026},"citing_paper":{"arxiv_id":"2605.03128","last_updated":"2026-06-10T19:08:48Z","snapshot_observed_at":"2026-08-14T19:55:26.214896Z","submitted_at":"2026-05-04T20:10:59Z","title":"Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-01T00:00:28.796229Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2605.03128"},"observation_digest":"sha256:5fc9c4e3749b6112581b26d3f227b02c65de6c92a455f42e6344e7e760ee620d","observation_id":"0567d58c-d3db-4df2-9a9d-a815d0c08c5c","resolution":{"observed_at":"2026-07-01T00:05:09.005116Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":"2601.03861","doi":"10.48550/arxiv.2601.03861","metadata_source":"pith","pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":"astro-ph.HE","work_id":"e22ac5d2-09e0-4a38-9d3b-9e086986e1bb","year":2026},"citing_paper":{"arxiv_id":"2605.20596","last_updated":"2026-05-20T01:07:52Z","snapshot_observed_at":"2026-08-03T00:01:05.266821Z","submitted_at":"2026-05-20T01:07:52Z","title":"Binary Neutron Star Merger Evolution and r-Process Enrichment in the Milky Way Disk","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-21T04:26:53.781342Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2605.20596"},"observation_digest":"sha256:c7407b57b508a619db9f6f229d142946241333627b660c6362a72e9150085fb4","observation_id":"21556dbe-e3fe-4ec1-abcc-bd676290df5f","resolution":{"observed_at":"2026-06-24T15:15:17.732011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-07-13T05:21:16.491609Z","title":"Pracchia and O","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.09109","last_updated":"2026-07-10T05:45:41Z","snapshot_observed_at":"2026-08-14T13:12:53.629328Z","submitted_at":"2026-07-10T05:45:41Z","title":"Fast Radio Bursts Trace Cosmic Star Formation with Little Delay","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-13T05:21:16.491609Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2607.09109"},"observation_digest":"sha256:c0568b752d9c22b2dd7ecce85820a7e67c9383f422fb5b8d5967e2f614bb5402","observation_id":"ea10e76e-5f77-4cbc-bf3f-38712baf1684","resolution":{"observed_at":"2026-07-13T05:21:16.491609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.03861","snapshot_observed_at":"2026-08-01T03:38:35.652761Z","title":"2026, arXiv e-prints, arXiv:2601.03861, doi: 10.48550/arXiv.2601.03861","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.23114","last_updated":"2026-07-25T09:00:22Z","snapshot_observed_at":"2026-08-14T00:46:11.535140Z","submitted_at":"2026-07-25T09:00:22Z","title":"Diverse Morphologies of GRB X-Ray Plateaus within a Common Magnetar Framework","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T03:38:35.652761Z"},"links":{"cited_paper":"/paper/2601.03861","citing_paper":"/paper/2607.23114"},"observation_digest":"sha256:37517ea943c14e62fe672980e1593f16d5328601291519712bff86f01952f2ea","observation_id":"f36a266d-bc2b-4bc7-a438-fae4efc339d8","resolution":{"observed_at":"2026-08-01T03:38:35.652761Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2601.03861/citation-record","integrity":"/paper/2601.03861/integrity","json":"/paper/2601.03861/citation-record.json","paper":"/paper/2601.03861"},"outbound":[],"paper":{"arxiv_id":"2601.03861","last_updated":"2026-08-05T10:16:47Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-08T23:09:13.622341Z","submitted_at":"2026-01-07T12:18:25Z","title":"Short gamma-ray burst progenitors have short delay times"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2601.03861."}