{"as_of":"2026-08-09T07:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4fd5feae82ac604ac599b6482fcb41fe40d8d60ce70e1caf71e0b6d532d52781","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":"2026-08-09T06:31:02.800959+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":"2026-08-08T13:33:06.253240Z","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":"1803.03410","last_updated":"2018-03-09T08:04:51Z","snapshot_observed_at":"2026-07-06T06:27:24.379369Z","submitted_at":"2018-03-09T08:04:51Z","title":"Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.03410","snapshot_observed_at":"2026-08-03T02:40:53.736725Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29650","last_updated":"2026-07-31T17:28:04Z","snapshot_observed_at":"2026-08-09T01:41:25.010948Z","submitted_at":"2026-07-31T17:28:04Z","title":"The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants","version":1},"reference_index":196,"source":"arxiv_source","source_observed_at":"2026-08-03T02:40:53.736725Z"},"links":{"cited_paper":"/paper/1803.03410","citing_paper":"/paper/2607.29650"},"observation_digest":"sha256:1a34bea3e595d03b180185bec8bf0f1a0c165e27d19c31e7414274e50e1a350c","observation_id":"8c732458-ab5d-4088-97ec-e734a47d2db8","resolution":{"observed_at":"2026-08-03T02:40:53.736725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.03410","last_updated":"2018-03-09T08:04:51Z","snapshot_observed_at":"2026-07-06T06:27:24.379369Z","submitted_at":"2018-03-09T08:04:51Z","title":"Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.03410","snapshot_observed_at":"2026-08-08T13:33:06.253240Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05421","last_updated":"2026-08-05T21:30:20Z","snapshot_observed_at":"2026-08-09T07:10:25.979343Z","submitted_at":"2026-08-05T21:30:20Z","title":"The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-08T13:33:06.253240Z"},"links":{"cited_paper":"/paper/1803.03410","citing_paper":"/paper/2608.05421"},"observation_digest":"sha256:4bc6ebc3253c0af8b4bd1ad1e527c120e5b9f400af23ac00d894b18968ecef9b","observation_id":"84235dfd-7f08-4c22-9182-7a9b1cc16b07","resolution":{"observed_at":"2026-08-08T13:33:06.253240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1803.03410/citation-record","integrity":"/paper/1803.03410/integrity","json":"/paper/1803.03410/citation-record.json","paper":"/paper/1803.03410"},"outbound":[],"paper":{"arxiv_id":"1803.03410","last_updated":"2018-03-09T08:04:51Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T06:27:24.379369Z","submitted_at":"2018-03-09T08:04:51Z","title":"Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing"},"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 2 inbound Pith citation observations for arXiv:1803.03410."}