{"as_of":"2026-08-06T18:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b10f16e9617320e675433ab6db49962546159a18aeac9ca94f26edd7f0f2c420","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":"2026-08-06T06:34:29.942622+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":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":184,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0906.0766","last_updated":"2009-06-03T20:33:05Z","snapshot_observed_at":"2026-07-06T01:53:58.307205Z","submitted_at":"2009-06-03T20:33:05Z","title":"Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission","version":1},"cited_work":{"arxiv_id":"0906.0766","doi":"10.1088/0004-637x/700/2/1589","metadata_source":"pith","pith_arxiv_id":"0906.0766","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission","venue":"astro-ph.SR","work_id":"55d43ad6-c658-4b6e-b951-aaf30e9572c0","year":2009},"citing_paper":{"arxiv_id":"2606.12034","last_updated":"2026-06-10T12:57:12Z","snapshot_observed_at":"2026-08-03T00:37:28.274620Z","submitted_at":"2026-06-10T12:57:12Z","title":"Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0906.0766","citing_paper":"/paper/2606.12034"},"observation_digest":"sha256:b8eeb405239b684788748d2c07d54439312578abea34c84f758553839a73edc7","observation_id":"523dd0e6-6471-4f5f-a22f-56c4ee0f0411","resolution":{"observed_at":"2026-06-28T03:31:30.923038Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0906.0766","last_updated":"2009-06-03T20:33:05Z","snapshot_observed_at":"2026-07-06T01:53:58.307205Z","submitted_at":"2009-06-03T20:33:05Z","title":"Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission","version":1},"cited_work":{"arxiv_id":"0906.0766","doi":"10.1088/0004-637x/700/2/1589","metadata_source":"pith","pith_arxiv_id":"0906.0766","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission","venue":"astro-ph.SR","work_id":"55d43ad6-c658-4b6e-b951-aaf30e9572c0","year":2009},"citing_paper":{"arxiv_id":"2606.25517","last_updated":"2026-06-24T07:50:04Z","snapshot_observed_at":"2026-08-02T20:21:05.194813Z","submitted_at":"2026-06-24T07:50:04Z","title":"Unveiling the nature of barium stars. I. Asteroseismic masses and the evolutionary link between Ba dwarfs and giants","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0906.0766","citing_paper":"/paper/2606.25517"},"observation_digest":"sha256:bc8aa7de19889f8ba15c15950738a0a4d643af48a7f5bdc610f86ec88787ca93","observation_id":"9476527b-4c4d-4dd2-ae5d-cfd2a7e30a82","resolution":{"observed_at":"2026-06-25T19:48:18.179395Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/0906.0766/citation-record","integrity":"/paper/0906.0766/integrity","json":"/paper/0906.0766/citation-record.json","paper":"/paper/0906.0766"},"outbound":[],"paper":{"arxiv_id":"0906.0766","last_updated":"2009-06-03T20:33:05Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T01:53:58.307205Z","submitted_at":"2009-06-03T20:33:05Z","title":"Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0906.0766."}