{"as_of":"2026-08-12T03:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9922b846e96338326b95be3abdd65d3a9c34339fb8bbdfdc32ea20b870165893","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:19:39.930647Z","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":"2006.14322","last_updated":"2020-07-29T11:26:56Z","snapshot_observed_at":"2026-08-11T14:31:37.928188Z","submitted_at":"2020-06-25T11:55:51Z","title":"Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.14322","snapshot_observed_at":"2026-08-06T18:16:14.828007Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08925","last_updated":"2025-07-11T18:00:00Z","snapshot_observed_at":"2026-08-06T21:48:06.406035Z","submitted_at":"2025-07-11T18:00:00Z","title":"Cosmological Simulations of Galaxies","version":1},"reference_index":234,"source":"arxiv_source","source_observed_at":"2026-08-06T18:16:14.828007Z"},"links":{"cited_paper":"/paper/2006.14322","citing_paper":"/paper/2507.08925"},"observation_digest":"sha256:92463b94b0e730a08f4018a2987ccba68c6a7283f6f857285b1a984047cc1488","observation_id":"64b50214-62e4-4558-91a0-b61376e47b92","resolution":{"observed_at":"2026-08-06T18:16:14.828007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.14322","last_updated":"2020-07-29T11:26:56Z","snapshot_observed_at":"2026-08-11T14:31:37.928188Z","submitted_at":"2020-06-25T11:55:51Z","title":"Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.14322","snapshot_observed_at":"2026-08-10T17:19:39.930647Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.06978","last_updated":"2026-08-07T08:55:46Z","snapshot_observed_at":"2026-08-12T03:10:47.019686Z","submitted_at":"2026-08-07T08:55:46Z","title":"Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-10T17:19:39.930647Z"},"links":{"cited_paper":"/paper/2006.14322","citing_paper":"/paper/2608.06978"},"observation_digest":"sha256:32a754636213cf78980df8d3b55f00a3bc442aa4f97c9ed1eea824668f42cb52","observation_id":"5f569694-dbf6-48ee-a670-7747e0627854","resolution":{"observed_at":"2026-08-10T17:19:39.930647Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2006.14322/citation-record","integrity":"/paper/2006.14322/integrity","json":"/paper/2006.14322/citation-record.json","paper":"/paper/2006.14322"},"outbound":[],"paper":{"arxiv_id":"2006.14322","last_updated":"2020-07-29T11:26:56Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-11T14:31:37.928188Z","submitted_at":"2020-06-25T11:55:51Z","title":"Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2006.14322."}