{"as_of":"2026-08-13T02:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0f4894e09e60b8e583576f39d8a841b368c1025a098ff3a8503281ca4e4e851f","coverage":[{"denominator":5,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T21:31:17.304399Z","state":"measured"},{"denominator":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-29T09:42:18.943460Z","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":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"cited_work":{"arxiv_id":"2602.20015","doi":"10.48550/arxiv.2602.20015","metadata_source":"arxiv_reference","pith_arxiv_id":"2602.20015","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"R., Dong, J., Huang, C","venue":"arXiv (Cornell University)","work_id":"806897c2-7d39-4c5b-b070-2e18cbde71cb","year":2026},"citing_paper":{"arxiv_id":"2605.28719","last_updated":"2026-05-27T16:39:15Z","snapshot_observed_at":"2026-07-06T23:38:14.056361Z","submitted_at":"2026-05-27T16:39:15Z","title":"A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$\\lambda$ Trends in Three Gas-Giant Mass Regimes","version":1},"reference_index":162,"source":"pdf_text","source_observed_at":"2026-06-29T09:42:18.943460Z"},"links":{"cited_paper":"/paper/2602.20015","citing_paper":"/paper/2605.28719"},"observation_digest":"sha256:150814035710d9d16772f93a70db836d8cf66de50038cc399d750c7b514cd845","observation_id":"c60375bb-1a89-43d0-98cf-2f4aaf79ea3a","resolution":{"observed_at":"2026-07-24T02:22:59.327324Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2602.20015/citation-record","integrity":"/paper/2602.20015/integrity","json":"/paper/2602.20015/citation-record.json","paper":"/paper/2602.20015"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T21:31:16.916622Z","title":"2020, AJ, 159, 123, doi: 10.3847/1538-3881/ab4fee Allard, F., Homeier, D., & Freytag, B","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-02T21:31:16.916622Z"},"links":{"citing_paper":"/paper/2602.20015"},"observation_digest":"sha256:70fd23682a3d32b98fb5b9050c6ce098bba88f74a30c9f63b3297bc812748edf","observation_id":"4e68c556-f912-444c-a486-2762e4332bbf","resolution":{"observed_at":"2026-08-02T21:31:16.916622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T21:31:17.069858Z","title":"Batygin, K., Bodenheimer, P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-02T21:31:17.069858Z"},"links":{"citing_paper":"/paper/2602.20015"},"observation_digest":"sha256:9050083f0353e5df1095892c99ee2def577a88e782f76b95cd87979e23ff8e47","observation_id":"9b663fd9-92fb-496d-8e98-fef2d083fe66","resolution":{"observed_at":"2026-08-02T21:31:17.069858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.10797","last_updated":"2024-02-22T10:58:50Z","snapshot_observed_at":"2026-08-09T23:16:22.188156Z","submitted_at":"2024-02-16T16:21:02Z","title":"BlackJAX: Composable Bayesian inference in JAX","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.10797","snapshot_observed_at":"2026-08-02T21:31:17.148021Z","title":"Cabezas, A., Corenflos, A., Lao, J., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-02T21:31:17.148021Z"},"links":{"cited_paper":"/paper/2402.10797","citing_paper":"/paper/2602.20015"},"observation_digest":"sha256:24e875fb9dbbfcfd348549b09363579af67ae85bdac73531a4839e6b6dd6163e","observation_id":"f8dffa7e-bf3e-497c-a1a9-ce5e9358fc3a","resolution":{"observed_at":"2026-08-02T21:31:17.148021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T21:31:17.225314Z","title":"Gilbert, G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-02T21:31:17.225314Z"},"links":{"citing_paper":"/paper/2602.20015"},"observation_digest":"sha256:32041ec8629948642fed324857c6b0e4b053bf8262c3fe3bb51841d160145188","observation_id":"59c9378e-3fba-43d4-b555-29a4f93dc74d","resolution":{"observed_at":"2026-08-02T21:31:17.225314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4246","last_updated":"2011-11-18T00:39:32Z","snapshot_observed_at":"2026-07-06T02:37:47.001497Z","submitted_at":"2011-11-18T00:39:32Z","title":"The No-U-Turn Sampler: Adaptively Setting Path Lengths in Hamiltonian Monte Carlo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.4246","snapshot_observed_at":"2026-08-02T21:31:17.304399Z","title":"Hoffman, M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-02T21:31:17.304399Z"},"links":{"cited_paper":"/paper/1111.4246","citing_paper":"/paper/2602.20015"},"observation_digest":"sha256:951e3dd03baeab7ce1c3a2393a24b52571aaef15e4235733f1c4571c6a2ea1be","observation_id":"ee2605b0-8690-4cc6-95c9-8f1ac6033d09","resolution":{"observed_at":"2026-08-02T21:31:17.304399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2602.20015","last_updated":"2026-07-23T05:12:01Z","latest_version":2,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-08T09:45:50.178707Z","submitted_at":"2026-02-23T16:22:06Z","title":"The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS"},"reference_resolution":{"displayed":5,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":5,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":5},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 1 inbound Pith citation observation for arXiv:2602.20015."}