{"as_of":"2026-08-07T20:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d0cbaf1f414a752dd180cf62fb3aaf8563b0f0b414b6ad2200346dd961321785","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":"2026-08-07T06:34:17.273281+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":"2026-08-01T00:42:46.093169Z","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":"2026-07-02T04:26:36.081650Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1105.0556","last_updated":"2011-05-26T16:20:53Z","snapshot_observed_at":"2026-07-06T02:27:12.427269Z","submitted_at":"2011-05-03T11:39:10Z","title":"Wind modelling of very massive stars up to 300 solar masses","version":2},"cited_work":{"arxiv_id":"1105.0556","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0556","snapshot_observed_at":"2026-07-02T04:26:36.081650Z","title":"Wind modelling of very massive stars up to 300 solar masses","venue":"astro-ph.SR","work_id":"14059d07-b66a-4c6d-8dc1-e3f83046c2fd","year":2011},"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":98,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1105.0556","citing_paper":"/paper/2606.02725"},"observation_digest":"sha256:81c4bae3f8ca19d9bc002d4cec80421e7fbe15a1b756a4e9e1b0b0e2e3bf98d9","observation_id":"3279a0c7-52f3-414f-b604-f1cc8cdcfffb","resolution":{"observed_at":"2026-06-28T13:02:10.596292Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0556","last_updated":"2011-05-26T16:20:53Z","snapshot_observed_at":"2026-07-06T02:27:12.427269Z","submitted_at":"2011-05-03T11:39:10Z","title":"Wind modelling of very massive stars up to 300 solar masses","version":2},"cited_work":{"arxiv_id":"1105.0556","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0556","snapshot_observed_at":"2026-07-02T04:26:36.081650Z","title":"Wind modelling of very massive stars up to 300 solar masses","venue":"astro-ph.SR","work_id":"14059d07-b66a-4c6d-8dc1-e3f83046c2fd","year":2011},"citing_paper":{"arxiv_id":"2606.03776","last_updated":"2026-06-02T15:28:50Z","snapshot_observed_at":"2026-07-06T23:44:00.144689Z","submitted_at":"2026-06-02T15:28:50Z","title":"Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-06-28T09:07:09.699995Z"},"links":{"cited_paper":"/paper/1105.0556","citing_paper":"/paper/2606.03776"},"observation_digest":"sha256:de03135d472fb78eeff4f76fe08446cd65802abfddb934c19447e38f8c0d6fbd","observation_id":"ff6a3ba5-a849-440e-842b-5e95b4e764f8","resolution":{"observed_at":"2026-07-02T04:26:36.082979Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0556","last_updated":"2011-05-26T16:20:53Z","snapshot_observed_at":"2026-07-06T02:27:12.427269Z","submitted_at":"2011-05-03T11:39:10Z","title":"Wind modelling of very massive stars up to 300 solar masses","version":2},"cited_work":{"arxiv_id":"1105.0556","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0556","snapshot_observed_at":"2026-07-02T04:26:36.081650Z","title":"Wind modelling of very massive stars up to 300 solar masses","venue":"astro-ph.SR","work_id":"14059d07-b66a-4c6d-8dc1-e3f83046c2fd","year":2011},"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":180,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1105.0556","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0d81afab89145c59b6b3fce9eeebb0de8996ece1cd33f08b4188716526e6b442","observation_id":"b15158e4-5c4a-4e43-8f5b-e48be0f0838b","resolution":{"observed_at":"2026-06-26T18:09:41.352457Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0556","last_updated":"2011-05-26T16:20:53Z","snapshot_observed_at":"2026-07-06T02:27:12.427269Z","submitted_at":"2011-05-03T11:39:10Z","title":"Wind modelling of very massive stars up to 300 solar masses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0556","snapshot_observed_at":"2026-08-01T00:42:46.093169Z","title":"A&A , keywords =","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":278,"source":"arxiv_source","source_observed_at":"2026-08-01T00:42:46.093169Z"},"links":{"cited_paper":"/paper/1105.0556","citing_paper":"/paper/2607.26147"},"observation_digest":"sha256:2e77cab52ee37c27d41a88d88267d529881c128f0024cbd9e5934464d8560b06","observation_id":"382ecbf2-cf94-4e78-84a7-919b60a37c36","resolution":{"observed_at":"2026-08-01T00:42:46.093169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1105.0556/citation-record","integrity":"/paper/1105.0556/integrity","json":"/paper/1105.0556/citation-record.json","paper":"/paper/1105.0556"},"outbound":[],"paper":{"arxiv_id":"1105.0556","last_updated":"2011-05-26T16:20:53Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T02:27:12.427269Z","submitted_at":"2011-05-03T11:39:10Z","title":"Wind modelling of very massive stars up to 300 solar masses"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1105.0556."}