{"as_of":"2026-08-11T06:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:029ed3b7bb7ba17137e72fa65a136fe7f9e696ba3270509ddfd77aaa5088c689","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":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":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T14:45:24.422607Z","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":6,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-09T14:45:24.422607Z","title":"doi:10.1093/mnras/stae2092","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01724","last_updated":"2025-02-03T19:00:00Z","snapshot_observed_at":"2026-08-10T16:39:22.557783Z","submitted_at":"2025-02-03T19:00:00Z","title":"Cosmic quenching","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-09T14:45:24.422607Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2502.01724"},"observation_digest":"sha256:9a7e5d304c23ea7788e752cac42134c8d219f349a4a08b9c0ece5db281b3a9cb","observation_id":"5746b549-8eb1-4554-8d7e-7f8c84e6bc11","resolution":{"observed_at":"2026-08-09T14:45:24.422607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":"2405.02242","doi":"10.48550/arxiv.2405.02242","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"C., Cullen, F., McLure, R","venue":"arXiv (Cornell University)","work_id":"1aafcc2a-0e48-432c-a4ff-500308f37537","year":2024},"citing_paper":{"arxiv_id":"2503.15313","last_updated":"2026-04-17T13:41:49Z","snapshot_observed_at":"2026-07-29T23:56:20.674056Z","submitted_at":"2025-03-19T15:27:08Z","title":"Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-22T23:40:38.874288Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2503.15313"},"observation_digest":"sha256:ab2d3a1fcc4711091433153bd9488bdd26176c600ed2b39d74e3b60c5f8dfc69","observation_id":"b3db56d2-9ecb-44a9-9ab0-1b9d113d9357","resolution":{"observed_at":"2026-05-22T23:42:16.285791Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":"2405.02242","doi":"10.48550/arxiv.2405.02242","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"C., Cullen, F., McLure, R","venue":"arXiv (Cornell University)","work_id":"1aafcc2a-0e48-432c-a4ff-500308f37537","year":2024},"citing_paper":{"arxiv_id":"2503.16596","last_updated":"2025-03-20T18:00:00Z","snapshot_observed_at":"2026-07-06T20:56:18.361337Z","submitted_at":"2025-03-20T18:00:00Z","title":"A \"Black Hole Star\" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-16T08:53:14.586891Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2503.16596"},"observation_digest":"sha256:cdc1817f9f4a07d9d7f28b3b6087bd94555b7ced2baf5d6f80258882f21b01ae","observation_id":"9e2dc0db-3b9a-467d-8b9d-6a4be16ccc77","resolution":{"observed_at":"2026-05-16T08:53:14.739514Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-06T22:10:20.073639Z","title":"C., Cullen , F., McLure , R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22642","last_updated":"2025-06-27T21:13:30Z","snapshot_observed_at":"2026-08-08T06:59:22.099443Z","submitted_at":"2025-06-27T21:13:30Z","title":"DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-06T22:10:20.073639Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2506.22642"},"observation_digest":"sha256:0dca56b9fd540da8b6c00e71865b13fe49c4fc265ec9b77f60a85cce961e4f40","observation_id":"f6926b01-3570-45b5-b471-2cc42b6b5066","resolution":{"observed_at":"2026-08-06T22:10:20.073639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":"2405.02242","doi":"10.48550/arxiv.2405.02242","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"C., Cullen, F., McLure, R","venue":"arXiv (Cornell University)","work_id":"1aafcc2a-0e48-432c-a4ff-500308f37537","year":2024},"citing_paper":{"arxiv_id":"2605.03000","last_updated":"2026-05-04T18:00:01Z","snapshot_observed_at":"2026-07-30T18:29:52.784345Z","submitted_at":"2026-05-04T18:00:01Z","title":"Are Nucleosynthetic Yields Universal? Interpreting the Multi-Elemental Abundances of Quiescent Galaxies over Cosmic Time Using Milky Way Stars","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-05-08T18:05:57.694517Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2605.03000"},"observation_digest":"sha256:f2ec9fe6128c1b4ad156886fb8a4b9ad2fb5a6386699f90c0c1fa16a1ce1098c","observation_id":"a2b1b153-2d28-4be7-94d9-08120db9fe28","resolution":{"observed_at":"2026-05-08T18:08:54.164588Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.02242","snapshot_observed_at":"2026-08-01T13:38:43.120172Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19057","last_updated":"2026-07-21T12:45:36Z","snapshot_observed_at":"2026-08-07T11:36:56.346856Z","submitted_at":"2026-07-21T12:45:36Z","title":"An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars","version":1},"reference_index":238,"source":"arxiv_source","source_observed_at":"2026-08-01T13:38:43.120172Z"},"links":{"cited_paper":"/paper/2405.02242","citing_paper":"/paper/2607.19057"},"observation_digest":"sha256:d553c74b54f2ed2171e7e9528f82c46cedc2a104d3f312898c5dbdfb1fc56726","observation_id":"d543f497-c29d-48c4-80d8-e78e9b2ca04f","resolution":{"observed_at":"2026-08-01T13:38:43.120172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2405.02242/citation-record","integrity":"/paper/2405.02242/integrity","json":"/paper/2405.02242/citation-record.json","paper":"/paper/2405.02242"},"outbound":[],"paper":{"arxiv_id":"2405.02242","last_updated":"2024-09-04T18:52:51Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T18:09:29.876755Z","submitted_at":"2024-05-03T16:53:09Z","title":"The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2405.02242."}