{"as_of":"2026-08-18T16:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bb25f3b9463d8d8fdb30cae3c8091d7ed53eaf8244fbc989746f28ebfede23d7","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":"2026-08-18T06:34:40.430872+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":"2026-08-11T17:51:31.552003Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":2,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.07893","last_updated":"2024-02-12T18:56:13Z","snapshot_observed_at":"2026-08-16T14:19:14.126211Z","submitted_at":"2024-02-12T18:56:13Z","title":"The TESS-Keck Survey XXI: 13 New Planets and Homogeneous Properties for 21 Subgiant Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07893","snapshot_observed_at":"2026-08-11T17:51:31.552003Z","title":"K., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08527","last_updated":"2024-12-11T16:38:31Z","snapshot_observed_at":"2026-08-17T10:59:50.287033Z","submitted_at":"2024-12-11T16:38:31Z","title":"Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-11T17:51:31.552003Z"},"links":{"cited_paper":"/paper/2402.07893","citing_paper":"/paper/2412.08527"},"observation_digest":"sha256:2b8f762bf9dccebc7bdbaa09c055dd28d2aa0eee8ab37cead9587a04fa29efdc","observation_id":"db289ac9-3e73-4a9b-b1bb-d1c4c9bb6384","resolution":{"observed_at":"2026-08-11T17:51:31.552003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07893","last_updated":"2024-02-12T18:56:13Z","snapshot_observed_at":"2026-08-16T14:19:14.126211Z","submitted_at":"2024-02-12T18:56:13Z","title":"The TESS-Keck Survey XXI: 13 New Planets and Homogeneous Properties for 21 Subgiant Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07893","snapshot_observed_at":"2026-08-10T20:19:17.763592Z","title":"K., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.08992","last_updated":"2025-01-15T18:16:42Z","snapshot_observed_at":"2026-08-12T22:22:01.683892Z","submitted_at":"2025-01-15T18:16:42Z","title":"Empirical Constraints on Tidal Dissipation in Exoplanet Host Stars","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T20:19:17.763592Z"},"links":{"cited_paper":"/paper/2402.07893","citing_paper":"/paper/2501.08992"},"observation_digest":"sha256:598a25b7b6aa37466151909d744ded66e294035b77674934f198c8192f72a308","observation_id":"7c8b3d98-d518-4d5e-adfb-3c192a55bfb8","resolution":{"observed_at":"2026-08-10T20:19:17.763592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07893","last_updated":"2024-02-12T18:56:13Z","snapshot_observed_at":"2026-08-16T14:19:14.126211Z","submitted_at":"2024-02-12T18:56:13Z","title":"The TESS-Keck Survey XXI: 13 New Planets and Homogeneous Properties for 21 Subgiant Systems","version":1},"cited_work":{"arxiv_id":"2402.07893","doi":"10.48550/arxiv.2402.07893","metadata_source":"arxiv_reference","pith_arxiv_id":"2402.07893","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"K., et al","venue":"arXiv (Cornell University)","work_id":"c84ad7b6-5869-458c-bd4d-e3ba1bc21fdb","year":2024},"citing_paper":{"arxiv_id":"2602.18553","last_updated":"2026-05-21T20:58:34Z","snapshot_observed_at":"2026-08-14T20:48:53.991745Z","submitted_at":"2026-02-20T19:00:00Z","title":"POSEIDON I: The Dynamical Origins of Transiting Neptunes","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-25T07:24:24.189406Z"},"links":{"cited_paper":"/paper/2402.07893","citing_paper":"/paper/2602.18553"},"observation_digest":"sha256:75767e5d00a65c2543b6d61f6d2136574781d58cf5a2ccea5d47e619a2e6393f","observation_id":"c7a6607b-8b61-4da7-8828-4405d38448f0","resolution":{"observed_at":"2026-05-25T07:25:28.106023Z","resolver_source":"arxiv_id","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":"2402.07893","last_updated":"2024-02-12T18:56:13Z","snapshot_observed_at":"2026-08-16T14:19:14.126211Z","submitted_at":"2024-02-12T18:56:13Z","title":"The TESS-Keck Survey XXI: 13 New Planets and Homogeneous Properties for 21 Subgiant Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07893","snapshot_observed_at":"2026-08-01T11:52:27.816769Z","title":"Gruppe/Group 6 Astronomy and Astrophysics","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19756","last_updated":"2026-07-22T05:01:51Z","snapshot_observed_at":"2026-08-05T03:29:27.369446Z","submitted_at":"2026-07-22T05:01:51Z","title":"CAFE follow-up of TESS hot Jupiter candidates left behind: I. Five newly confirmed planets and a false positive","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T11:52:27.816769Z"},"links":{"cited_paper":"/paper/2402.07893","citing_paper":"/paper/2607.19756"},"observation_digest":"sha256:494b44c6d8338e0858884d426902e7d8da60f3a24a15b6315d09983e609d6a9f","observation_id":"245ce521-d53a-42bb-8138-d5ef01089a7d","resolution":{"observed_at":"2026-08-01T11:52:27.816769Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2402.07893/citation-record","integrity":"/paper/2402.07893/integrity","json":"/paper/2402.07893/citation-record.json","paper":"/paper/2402.07893"},"outbound":[],"paper":{"arxiv_id":"2402.07893","last_updated":"2024-02-12T18:56:13Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-16T14:19:14.126211Z","submitted_at":"2024-02-12T18:56:13Z","title":"The TESS-Keck Survey XXI: 13 New Planets and Homogeneous Properties for 21 Subgiant Systems"},"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 4 inbound Pith citation observations for arXiv:2402.07893."}