{"as_of":"2026-08-12T23:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b9307e558dd7d1669f65938b0c648f406b6e8c037f45dcf5e4fd1f468e400e61","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T14:01:38.526881Z","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":"2026-06-28T13:02:10.909651Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0803.0866","last_updated":"2008-03-06T13:48:14Z","snapshot_observed_at":"2026-08-11T16:15:12.217622Z","submitted_at":"2008-03-06T13:48:14Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0866","snapshot_observed_at":"2026-08-11T14:01:38.526881Z","title":"title Mass loss from late-type WN stars and its Z-dependence","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.12534","last_updated":"2024-12-17T04:48:44Z","snapshot_observed_at":"2026-08-11T21:05:06.173587Z","submitted_at":"2024-12-17T04:48:44Z","title":"Wolf-Rayet Colliding Wind Binaries","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-11T14:01:38.526881Z"},"links":{"cited_paper":"/paper/0803.0866","citing_paper":"/paper/2412.12534"},"observation_digest":"sha256:3d984595ba775f7c30edc09e0c6971684d8f204ce5c143f0e14899a33a7c2c16","observation_id":"9db45750-a8eb-4c41-bde4-5b09c736c197","resolution":{"observed_at":"2026-08-11T14:01:38.526881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0866","last_updated":"2008-03-06T13:48:14Z","snapshot_observed_at":"2026-08-11T16:15:12.217622Z","submitted_at":"2008-03-06T13:48:14Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","version":1},"cited_work":{"arxiv_id":"0803.0866","doi":null,"metadata_source":"pith","pith_arxiv_id":"0803.0866","snapshot_observed_at":"2026-06-28T13:02:10.909651Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","venue":"astro-ph","work_id":"7d4002d3-305b-49f7-bffe-3710de7c96e6","year":2008},"citing_paper":{"arxiv_id":"2606.02725","last_updated":"2026-06-01T18:00:08Z","snapshot_observed_at":"2026-08-05T14:45:05.891181Z","submitted_at":"2026-06-01T18:00:08Z","title":"Can current models predict the local black hole merger rate?","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0803.0866","citing_paper":"/paper/2606.02725"},"observation_digest":"sha256:326b5991df85c879ec051a1a7aeec4b7ed4ffba532a61afba6dd54ac1261ea4b","observation_id":"e98421bb-5947-4210-b71b-4737704c3620","resolution":{"observed_at":"2026-06-28T13:02:10.910902Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0866","last_updated":"2008-03-06T13:48:14Z","snapshot_observed_at":"2026-08-11T16:15:12.217622Z","submitted_at":"2008-03-06T13:48:14Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","version":1},"cited_work":{"arxiv_id":"0803.0866","doi":null,"metadata_source":"pith","pith_arxiv_id":"0803.0866","snapshot_observed_at":"2026-06-28T13:02:10.909651Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","venue":"astro-ph","work_id":"7d4002d3-305b-49f7-bffe-3710de7c96e6","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":181,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0803.0866","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:1c755d194c3ace84f93b98cc163856299aa1162f39ee1f1d7d8bd145886cf643","observation_id":"20d3911f-670a-4e98-8347-17bfed75eb0d","resolution":{"observed_at":"2026-06-26T18:09:41.735466Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0866","last_updated":"2008-03-06T13:48:14Z","snapshot_observed_at":"2026-08-11T16:15:12.217622Z","submitted_at":"2008-03-06T13:48:14Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0866","snapshot_observed_at":"2026-08-01T00:42:41.607972Z","title":"Very massive stars approaching the Eddington limit","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.26147","last_updated":"2026-07-28T18:00:30Z","snapshot_observed_at":"2026-08-07T18:22:27.355170Z","submitted_at":"2026-07-28T18:00:30Z","title":"The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity","version":1},"reference_index":236,"source":"arxiv_source","source_observed_at":"2026-08-01T00:42:41.607972Z"},"links":{"cited_paper":"/paper/0803.0866","citing_paper":"/paper/2607.26147"},"observation_digest":"sha256:4966ceef9604f8caaa198bcabcdda53dfb817537a052b02755bdfd854471b2bc","observation_id":"63cbd4c1-846b-43de-9380-0f8329388ded","resolution":{"observed_at":"2026-08-01T00:42:41.607972Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/0803.0866/citation-record","integrity":"/paper/0803.0866/integrity","json":"/paper/0803.0866/citation-record.json","paper":"/paper/0803.0866"},"outbound":[],"paper":{"arxiv_id":"0803.0866","last_updated":"2008-03-06T13:48:14Z","latest_version":1,"primary_category":"astro-ph","snapshot_observed_at":"2026-08-11T16:15:12.217622Z","submitted_at":"2008-03-06T13:48:14Z","title":"Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:0803.0866."}