{"as_of":"2026-08-18T13:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8d38cf449332a59987b87bb1a6d98ef7b00510bfe6bf8e7933c67dcd33fddd8f","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":"2026-08-18T06:34:40.430872+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":"2026-08-15T14:18:44.452350Z","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":"2026-08-12T12:11:58.180000Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2201.02458","last_updated":"2022-01-07T14:08:14Z","snapshot_observed_at":"2026-08-18T08:15:59.842728Z","submitted_at":"2022-01-07T14:08:14Z","title":"Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures","version":1},"cited_work":{"arxiv_id":"2201.02458","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.02458","snapshot_observed_at":"2026-08-12T12:11:58.180000Z","title":"Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures","venue":"astro-ph.SR","work_id":"e74f6be1-77bd-4a03-8164-754660c8fde4","year":2022},"citing_paper":{"arxiv_id":"2608.11010","last_updated":"2026-08-12T11:49:27Z","snapshot_observed_at":"2026-08-18T07:54:18.458089Z","submitted_at":"2026-08-11T14:56:32Z","title":"Gravity modes and potential evidence for Rossby Waves in late O-type supergiants","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-12T12:11:53.921507Z"},"links":{"cited_paper":"/paper/2201.02458","citing_paper":"/paper/2608.11010"},"observation_digest":"sha256:2f6872559d401f22381faacf623d5aecd4165b6c9042d98f8c557338542180b2","observation_id":"c14a6896-1ac7-49fd-bc6d-7a8487a28a55","resolution":{"observed_at":"2026-08-12T12:11:58.192188Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02458","last_updated":"2022-01-07T14:08:14Z","snapshot_observed_at":"2026-08-18T08:15:59.842728Z","submitted_at":"2022-01-07T14:08:14Z","title":"Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.02458","snapshot_observed_at":"2026-08-15T14:18:44.452350Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11010","last_updated":"2026-08-12T11:49:27Z","snapshot_observed_at":"2026-08-18T07:54:18.458089Z","submitted_at":"2026-08-11T14:56:32Z","title":"Gravity modes and potential evidence for Rossby Waves in late O-type supergiants","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T14:18:44.452350Z"},"links":{"cited_paper":"/paper/2201.02458","citing_paper":"/paper/2608.11010"},"observation_digest":"sha256:2e882dbf6ac9930b7c0421f424b96cc6196720bdfc4d14c8087d0b31dffa25a9","observation_id":"0e1b9e83-6075-4e15-9b33-2b32b28982a8","resolution":{"observed_at":"2026-08-15T14:18:44.452350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2201.02458/citation-record","integrity":"/paper/2201.02458/integrity","json":"/paper/2201.02458/citation-record.json","paper":"/paper/2201.02458"},"outbound":[],"paper":{"arxiv_id":"2201.02458","last_updated":"2022-01-07T14:08:14Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-18T08:15:59.842728Z","submitted_at":"2022-01-07T14:08:14Z","title":"Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2201.02458."}