{"as_of":"2026-08-07T05:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c917250e6ee57d42027c4ac77e656c258fb25ec5bd12af455dc64f7c4fccdc02","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":"2026-08-06T06:34:29.942622+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":"2026-08-06T18:36:06.295407Z","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":3,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2409.05716","last_updated":"2025-06-26T17:02:47Z","snapshot_observed_at":"2026-07-06T19:12:36.212757Z","submitted_at":"2024-09-09T15:25:53Z","title":"Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.05716","snapshot_observed_at":"2026-08-06T18:36:06.295407Z","title":"Salcido and I.G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.07991","last_updated":"2025-07-10T17:59:06Z","snapshot_observed_at":"2026-08-06T18:25:29.640613Z","submitted_at":"2025-07-10T17:59:06Z","title":"Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T18:36:06.295407Z"},"links":{"cited_paper":"/paper/2409.05716","citing_paper":"/paper/2507.07991"},"observation_digest":"sha256:544da095c1512339f24081a31dd833be61490d91253a4aea46609c88e4f2e2f7","observation_id":"10b041f2-9e41-4cb7-85c1-b358e94c7bab","resolution":{"observed_at":"2026-08-06T18:36:06.295407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.05716","last_updated":"2025-06-26T17:02:47Z","snapshot_observed_at":"2026-07-06T19:12:36.212757Z","submitted_at":"2024-09-09T15:25:53Z","title":"Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters","version":3},"cited_work":{"arxiv_id":"2409.05716","doi":"10.48550/arxiv.2409.05716","metadata_source":"arxiv_reference","pith_arxiv_id":"2409.05716","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Salcido and I","venue":"arXiv (Cornell University)","work_id":"144a074e-6895-4cd1-b494-812c9db20cb2","year":2025},"citing_paper":{"arxiv_id":"2604.19744","last_updated":"2026-04-21T17:59:26Z","snapshot_observed_at":"2026-07-31T18:40:46.399244Z","submitted_at":"2026-04-21T17:59:26Z","title":"Precision Kinematic Sunyaev--Zel'dovich Measurements Across Halo Mass and Redshift with DESI DR2 and ACT DR6: Part I. Luminous Red Galaxies","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-10T01:27:17.997565Z"},"links":{"cited_paper":"/paper/2409.05716","citing_paper":"/paper/2604.19744"},"observation_digest":"sha256:d07bb7b44b969cea9a09506c65ea68f7445a2cc1ef4ac05c77f240122b9d9c08","observation_id":"42508a82-87cb-4808-86dd-0fafa7464878","resolution":{"observed_at":"2026-05-11T13:36:06.724352Z","resolver_source":"arxiv_id","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":"2409.05716","last_updated":"2025-06-26T17:02:47Z","snapshot_observed_at":"2026-07-06T19:12:36.212757Z","submitted_at":"2024-09-09T15:25:53Z","title":"Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters","version":3},"cited_work":{"arxiv_id":"2409.05716","doi":"10.48550/arxiv.2409.05716","metadata_source":"arxiv_reference","pith_arxiv_id":"2409.05716","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Salcido and I","venue":"arXiv (Cornell University)","work_id":"144a074e-6895-4cd1-b494-812c9db20cb2","year":2025},"citing_paper":{"arxiv_id":"2606.27714","last_updated":"2026-06-26T04:44:56Z","snapshot_observed_at":"2026-08-01T17:32:21.309572Z","submitted_at":"2026-06-26T04:44:56Z","title":"Fast Radio Bursts as Cosmological Probes","version":1},"reference_index":170,"source":"arxiv_source","source_observed_at":"2026-06-29T03:50:16.999402Z"},"links":{"cited_paper":"/paper/2409.05716","citing_paper":"/paper/2606.27714"},"observation_digest":"sha256:bd16105f83f84245af64b98a2b1f8ae7357ba6aa186647d41ecc89ff4c12f5ed","observation_id":"9a448665-73ca-432f-89a6-803c27f7e145","resolution":{"observed_at":"2026-06-29T03:53:05.201186Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"2409.05716","last_updated":"2025-06-26T17:02:47Z","snapshot_observed_at":"2026-07-06T19:12:36.212757Z","submitted_at":"2024-09-09T15:25:53Z","title":"Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.05716","snapshot_observed_at":"2026-08-03T13:53:50.356451Z","title":"McCarthy","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.29091","last_updated":"2026-07-31T07:17:11Z","snapshot_observed_at":"2026-08-05T23:12:35.807552Z","submitted_at":"2026-07-31T07:17:11Z","title":"Direct shear $\\times$ kSZ correlation: controlling baryons without modeling galaxies","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T13:53:50.356451Z"},"links":{"cited_paper":"/paper/2409.05716","citing_paper":"/paper/2607.29091"},"observation_digest":"sha256:7feb47fdddbf378cd7a5784f03b796a27e66c1bc40e17f55601a7a94629aa43d","observation_id":"e97b79cb-dd32-4688-909b-7e20b9f31e09","resolution":{"observed_at":"2026-08-03T13:53:50.356451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2409.05716/citation-record","integrity":"/paper/2409.05716/integrity","json":"/paper/2409.05716/citation-record.json","paper":"/paper/2409.05716"},"outbound":[],"paper":{"arxiv_id":"2409.05716","last_updated":"2025-06-26T17:02:47Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T19:12:36.212757Z","submitted_at":"2024-09-09T15:25:53Z","title":"Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters"},"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 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2409.05716."}