{"as_of":"2026-08-09T07:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:64ab58b48e51838bd9aff3f6922bc3abcdcf773f3627efe515305898f7b74b12","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+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":"2026-08-07T20:40:57.142809Z","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":"1402.3616","last_updated":"2014-02-14T23:00:49Z","snapshot_observed_at":"2026-07-06T03:36:03.241855Z","submitted_at":"2014-02-14T23:00:49Z","title":"High proper motion X-ray binaries from the Yale Southern Proper Motion Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.3616","snapshot_observed_at":"2026-08-07T20:40:57.142809Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05946","last_updated":"2026-08-06T12:13:20Z","snapshot_observed_at":"2026-08-09T07:11:57.724361Z","submitted_at":"2026-08-06T12:13:20Z","title":"Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-07T20:40:57.142809Z"},"links":{"cited_paper":"/paper/1402.3616","citing_paper":"/paper/2608.05946"},"observation_digest":"sha256:ca4a191770fe3355cde3e9aa20816352da332a2766ea0cdffc90a79fdf9c0885","observation_id":"fe8a84d8-fcce-4695-8a7a-14179cb9dc5d","resolution":{"observed_at":"2026-08-07T20:40:57.142809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1402.3616/citation-record","integrity":"/paper/1402.3616/integrity","json":"/paper/1402.3616/citation-record.json","paper":"/paper/1402.3616"},"outbound":[],"paper":{"arxiv_id":"1402.3616","last_updated":"2014-02-14T23:00:49Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T03:36:03.241855Z","submitted_at":"2014-02-14T23:00:49Z","title":"High proper motion X-ray binaries from the Yale Southern Proper Motion Survey"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1402.3616."}