{"as_of":"2026-08-15T18:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:06dab62cd378d91bcdd04eec3f44e4a2b15d3ef0c740dd79e21ef884bcf06b0a","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":"2026-08-14T11:35:56.112922Z","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":"2026-05-22T09:31:21.108522Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1107.4106","last_updated":"2011-10-17T11:58:30Z","snapshot_observed_at":"2026-08-15T07:24:54.081449Z","submitted_at":"2011-07-20T20:15:13Z","title":"The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.4106","snapshot_observed_at":"2026-08-14T11:35:56.112922Z","title":"Belczynski, T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.08822","last_updated":"2019-12-09T07:53:33Z","snapshot_observed_at":"2026-08-15T12:42:26.082822Z","submitted_at":"2019-08-23T13:39:38Z","title":"Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:35:56.112922Z"},"links":{"cited_paper":"/paper/1107.4106","citing_paper":"/paper/1908.08822"},"observation_digest":"sha256:04d4f2ad9c0c797e78c376b953fe2b2f3bdedabaa5becba94884a76dbd65bad5","observation_id":"f63c0e81-6c63-41b7-891b-b0e3ad2e5e51","resolution":{"observed_at":"2026-08-14T11:35:56.112922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4106","last_updated":"2011-10-17T11:58:30Z","snapshot_observed_at":"2026-08-15T07:24:54.081449Z","submitted_at":"2011-07-20T20:15:13Z","title":"The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate","version":2},"cited_work":{"arxiv_id":"1107.4106","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.4106","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate","venue":"astro-ph.GA","work_id":"b348d57c-68d3-4d3b-89ff-996cce73401b","year":2011},"citing_paper":{"arxiv_id":"2605.21580","last_updated":"2026-05-20T18:00:01Z","snapshot_observed_at":"2026-08-14T23:17:43.350104Z","submitted_at":"2026-05-20T18:00:01Z","title":"Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions","version":1},"reference_index":160,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1107.4106","citing_paper":"/paper/2605.21580"},"observation_digest":"sha256:276019e9e27db5de8c42e0eef7ca5ce83cd74d1066f606a339829aa6a9786d21","observation_id":"88a6ac2b-dc3b-496d-9875-b79edeb9f2f1","resolution":{"observed_at":"2026-05-22T09:31:21.110952Z","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/1107.4106/citation-record","integrity":"/paper/1107.4106/integrity","json":"/paper/1107.4106/citation-record.json","paper":"/paper/1107.4106"},"outbound":[],"paper":{"arxiv_id":"1107.4106","last_updated":"2011-10-17T11:58:30Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-15T07:24:54.081449Z","submitted_at":"2011-07-20T20:15:13Z","title":"The fate of Cyg X-1: an empirical lower limit on BH-NS merger rate"},"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:1107.4106."}