{"as_of":"2026-08-08T22:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5b3d7b522f2a0cd460422a639507e38c6ca2e981424cc21b7c3b61f5a846e7c8","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":"2026-08-08T06:32:00.761636+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":"2026-08-05T20:04:16.086649Z","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":"2026-07-12T07:08:35.622816Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0909.3585","last_updated":"2009-09-19T13:36:54Z","snapshot_observed_at":"2026-07-06T01:57:49.894336Z","submitted_at":"2009-09-19T13:36:54Z","title":"Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars","version":1},"cited_work":{"arxiv_id":"0909.3585","doi":null,"metadata_source":"pith","pith_arxiv_id":"0909.3585","snapshot_observed_at":"2026-07-12T07:08:35.622816Z","title":"Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars","venue":"astro-ph.SR","work_id":"c9314ca0-240f-4399-834b-1266f9643868","year":2009},"citing_paper":{"arxiv_id":"2607.02775","last_updated":"2026-07-02T21:15:13Z","snapshot_observed_at":"2026-08-06T17:09:51.786473Z","submitted_at":"2026-07-02T21:15:13Z","title":"The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-12T07:07:35.219491Z"},"links":{"cited_paper":"/paper/0909.3585","citing_paper":"/paper/2607.02775"},"observation_digest":"sha256:0ab7339ca125bf64e3d7eaa6d0318f406113e688a8c05ac90701d1b51fdbf984","observation_id":"3959235f-9509-4453-8c84-4f8e0d9b40b8","resolution":{"observed_at":"2026-07-12T07:08:35.624933Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3585","last_updated":"2009-09-19T13:36:54Z","snapshot_observed_at":"2026-07-06T01:57:49.894336Z","submitted_at":"2009-09-19T13:36:54Z","title":"Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3585","snapshot_observed_at":"2026-08-05T20:04:16.086649Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.03383","last_updated":"2026-08-04T09:32:24Z","snapshot_observed_at":"2026-08-07T23:10:59.919361Z","submitted_at":"2026-08-04T09:32:24Z","title":"The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-05T20:04:16.086649Z"},"links":{"cited_paper":"/paper/0909.3585","citing_paper":"/paper/2608.03383"},"observation_digest":"sha256:fb5c67f406024f15a3b8f1cbbb4df5f922e0bdb56b77ab9b454e1c390eec54ea","observation_id":"f06ec259-1b0c-4271-bade-6dc5dd1c4b30","resolution":{"observed_at":"2026-08-05T20:04:16.086649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/0909.3585/citation-record","integrity":"/paper/0909.3585/integrity","json":"/paper/0909.3585/citation-record.json","paper":"/paper/0909.3585"},"outbound":[],"paper":{"arxiv_id":"0909.3585","last_updated":"2009-09-19T13:36:54Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T01:57:49.894336Z","submitted_at":"2009-09-19T13:36:54Z","title":"Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0909.3585."}