{"as_of":"2026-08-15T23:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:58ec91c56376bddef5005ed92f416367cb2bb5b6b2f5cc949b678d0bf690aa4b","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":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":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:35:56.122900Z","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":"2026-06-28T13:02:10.520462Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1705.04734","last_updated":"2017-05-11T17:59:59Z","snapshot_observed_at":"2026-08-14T23:59:14.777634Z","submitted_at":"2017-05-11T17:59:59Z","title":"Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.04734","snapshot_observed_at":"2026-08-14T11:35:56.122900Z","title":"Marchant, N","venue":null,"work_id":null,"year":2017},"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":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:35:56.122900Z"},"links":{"cited_paper":"/paper/1705.04734","citing_paper":"/paper/1908.08822"},"observation_digest":"sha256:2a574fce856610d7a753153bdc566566bc47a722282af6a75b03b88e5b67eff3","observation_id":"9acfd91e-e501-4c6f-97ea-15cc1b89a1a8","resolution":{"observed_at":"2026-08-14T11:35:56.122900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.04734","last_updated":"2017-05-11T17:59:59Z","snapshot_observed_at":"2026-08-14T23:59:14.777634Z","submitted_at":"2017-05-11T17:59:59Z","title":"Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.04734","snapshot_observed_at":"2026-08-09T04:41:35.785289Z","title":"title Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03523","last_updated":"2025-08-13T14:42:57Z","snapshot_observed_at":"2026-08-14T19:42:33.711846Z","submitted_at":"2025-02-05T19:00:01Z","title":"Population Synthesis of Gravitational Wave Sources","version":2},"reference_index":152,"source":"arxiv_source","source_observed_at":"2026-08-09T04:41:35.785289Z"},"links":{"cited_paper":"/paper/1705.04734","citing_paper":"/paper/2502.03523"},"observation_digest":"sha256:5f320f63f5cf67590093b20a21436c9e4a935b95286dfa3f096f014321b6bc93","observation_id":"eb898c42-81f9-4176-b407-4f74e04b8cf4","resolution":{"observed_at":"2026-08-09T04:41:35.785289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.04734","last_updated":"2017-05-11T17:59:59Z","snapshot_observed_at":"2026-08-14T23:59:14.777634Z","submitted_at":"2017-05-11T17:59:59Z","title":"Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity","version":1},"cited_work":{"arxiv_id":"1705.04734","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.04734","snapshot_observed_at":"2026-06-28T13:02:10.520462Z","title":"Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity","venue":"astro-ph.HE","work_id":"37c6f7eb-0310-474a-9a13-8f279c6c24cb","year":2017},"citing_paper":{"arxiv_id":"2606.02725","last_updated":"2026-06-01T18:00:08Z","snapshot_observed_at":"2026-08-13T17:30:50.157815Z","submitted_at":"2026-06-01T18:00:08Z","title":"Can current models predict the local black hole merger rate?","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1705.04734","citing_paper":"/paper/2606.02725"},"observation_digest":"sha256:27207284200a89c96c6ed599a84e8260c09aa09e6c2935a40d78936352833fb9","observation_id":"850e876d-4587-49c9-aafe-a5b1c6fd4229","resolution":{"observed_at":"2026-06-28T13:02:10.521782Z","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/1705.04734/citation-record","integrity":"/paper/1705.04734/integrity","json":"/paper/1705.04734/citation-record.json","paper":"/paper/1705.04734"},"outbound":[],"paper":{"arxiv_id":"1705.04734","last_updated":"2017-05-11T17:59:59Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T23:59:14.777634Z","submitted_at":"2017-05-11T17:59:59Z","title":"Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity"},"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 3 inbound Pith citation observations for arXiv:1705.04734."}