{"as_of":"2026-08-21T02:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f654007bd9c724a524990fddf1c48edf0d902ee60fae65af87cf4a1642dce0c9","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":"2026-08-20T06:33:59.587034+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":"2026-08-02T21:01:56.393708Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T15:29:56.578473Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2403.19236","last_updated":"2024-12-09T19:14:26Z","snapshot_observed_at":"2026-08-16T14:05:37.304116Z","submitted_at":"2024-03-28T08:47:51Z","title":"Measuring the baryon fraction using galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.19236","snapshot_observed_at":"2026-08-02T21:01:56.393708Z","title":"Krolewski and W","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.21733","last_updated":"2026-06-28T15:46:45Z","snapshot_observed_at":"2026-08-15T18:19:32.462703Z","submitted_at":"2026-02-25T09:43:05Z","title":"A sound horizon independent measurement of $H_0$ from BOSS, DESI and DES Y3","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-02T21:01:56.393708Z"},"links":{"cited_paper":"/paper/2403.19236","citing_paper":"/paper/2602.21733"},"observation_digest":"sha256:b55a232f120d24ebaba246563f39b497f352ee91507486a43e9a8654d3931ee5","observation_id":"9e702ed2-552c-42f0-87fb-7ecf8db8d7e1","resolution":{"observed_at":"2026-08-02T21:01:56.393708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.19236","last_updated":"2024-12-09T19:14:26Z","snapshot_observed_at":"2026-08-16T14:05:37.304116Z","submitted_at":"2024-03-28T08:47:51Z","title":"Measuring the baryon fraction using galaxy clustering","version":2},"cited_work":{"arxiv_id":"2403.19236","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2403.19236","snapshot_observed_at":"2026-07-04T15:29:56.578473Z","title":"Krolewski and W","venue":null,"work_id":"033a18cf-e461-41a8-95cb-364f0804f41a","year":2025},"citing_paper":{"arxiv_id":"2605.06267","last_updated":"2026-05-07T13:43:27Z","snapshot_observed_at":"2026-08-18T20:22:07.247825Z","submitted_at":"2026-05-07T13:43:27Z","title":"Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-08T05:39:03.436269Z"},"links":{"cited_paper":"/paper/2403.19236","citing_paper":"/paper/2605.06267"},"observation_digest":"sha256:46a140c1b4aaa9a88c1dc868978b3cb913f4ee08f19fa4902a22483bde2950a8","observation_id":"7bbab48c-8915-456a-9724-b8520117ebfc","resolution":{"observed_at":"2026-05-11T21:26:14.034167Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.19236","last_updated":"2024-12-09T19:14:26Z","snapshot_observed_at":"2026-08-16T14:05:37.304116Z","submitted_at":"2024-03-28T08:47:51Z","title":"Measuring the baryon fraction using galaxy clustering","version":2},"cited_work":{"arxiv_id":"2403.19236","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2403.19236","snapshot_observed_at":"2026-07-04T15:29:56.578473Z","title":"Krolewski and W","venue":null,"work_id":"033a18cf-e461-41a8-95cb-364f0804f41a","year":2025},"citing_paper":{"arxiv_id":"2606.26237","last_updated":"2026-06-24T18:00:03Z","snapshot_observed_at":"2026-07-07T00:00:36.766142Z","submitted_at":"2026-06-24T18:00:03Z","title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","version":1},"reference_index":214,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2403.19236","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:8362166920c529e8da174259833d32d8fab855f6cff3ad3f898c329e1ea78826","observation_id":"cc6e3893-4a4c-4ef0-9c41-16ba2f8163f0","resolution":{"observed_at":"2026-07-04T15:29:56.580648Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.19236","last_updated":"2024-12-09T19:14:26Z","snapshot_observed_at":"2026-08-16T14:05:37.304116Z","submitted_at":"2024-03-28T08:47:51Z","title":"Measuring the baryon fraction using galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.19236","snapshot_observed_at":"2026-07-11T07:11:58.504385Z","title":"Krolewski and W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.05367","last_updated":"2026-07-06T17:45:50Z","snapshot_observed_at":"2026-08-14T08:25:34.980202Z","submitted_at":"2026-07-06T17:45:50Z","title":"Investigating a Possible Variation of the Gravitational Constant Through Gas Mass Fraction Measurements and Type Ia Supernovae Observations","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-11T07:11:58.504385Z"},"links":{"cited_paper":"/paper/2403.19236","citing_paper":"/paper/2607.05367"},"observation_digest":"sha256:9554371c843c9f9ad3c35e15e45933ff7a713047233d7426e460223a2ced78f9","observation_id":"7963fe74-c0eb-4004-b528-92da66566d7b","resolution":{"observed_at":"2026-07-11T07:11:58.504385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2403.19236/citation-record","integrity":"/paper/2403.19236/integrity","json":"/paper/2403.19236/citation-record.json","paper":"/paper/2403.19236"},"outbound":[],"paper":{"arxiv_id":"2403.19236","last_updated":"2024-12-09T19:14:26Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T14:05:37.304116Z","submitted_at":"2024-03-28T08:47:51Z","title":"Measuring the baryon fraction using galaxy clustering"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2403.19236."}