{"as_of":"2026-08-23T12:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:721d4f4fb2c41939206f5fb7eacdcd8bd4480ac27afa5b564a11e46a15e47d35","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+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":"2026-07-13T06:20:04.707661Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.17368","last_updated":"2024-07-25T10:52:36Z","snapshot_observed_at":"2026-08-16T13:57:33.915798Z","submitted_at":"2024-04-26T12:41:42Z","title":"Inefficient star formation in high Mach number environments I. The turbulent support analytical model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.17368","snapshot_observed_at":"2026-07-13T06:20:04.707661Z","title":"The turbulent support analytical model","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.08846","last_updated":"2026-07-09T18:11:36Z","snapshot_observed_at":"2026-08-17T04:17:42.426140Z","submitted_at":"2026-07-09T18:11:36Z","title":"mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-13T06:20:04.707661Z"},"links":{"cited_paper":"/paper/2404.17368","citing_paper":"/paper/2607.08846"},"observation_digest":"sha256:fca4ce092b9bf61adb7a129f4772fe12d802c92c5b4d0f451fb6b468b0e1c219","observation_id":"c92ae9af-0a5d-41e8-9a4e-fe84f1c4ebe5","resolution":{"observed_at":"2026-07-13T06:20:04.707661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.17368/citation-record","integrity":"/paper/2404.17368/integrity","json":"/paper/2404.17368/citation-record.json","paper":"/paper/2404.17368"},"outbound":[],"paper":{"arxiv_id":"2404.17368","last_updated":"2024-07-25T10:52:36Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T13:57:33.915798Z","submitted_at":"2024-04-26T12:41:42Z","title":"Inefficient star formation in high Mach number environments I. The turbulent support analytical model"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2404.17368."}