{"as_of":"2026-08-13T10:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:322dd9368f90f0f826e5b012f9e755cd484e754999edfbc798605e89d6014bd5","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":"2026-08-13T06:32:02.005865+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":"2026-06-27T21:13:45.849333Z","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":"2026-07-02T19:57:19.631478Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2204.05316","last_updated":"2022-12-14T00:39:55Z","snapshot_observed_at":"2026-07-06T12:59:16.136198Z","submitted_at":"2022-04-11T18:00:00Z","title":"Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics","version":2},"cited_work":{"arxiv_id":"2204.05316","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.05316","snapshot_observed_at":"2026-07-02T19:57:19.631478Z","title":null,"venue":null,"work_id":"1cce748e-ce89-4343-a23e-674ab15d6757","year":null},"citing_paper":{"arxiv_id":"2606.07741","last_updated":"2026-06-05T18:00:02Z","snapshot_observed_at":"2026-07-06T23:47:19.773490Z","submitted_at":"2026-06-05T18:00:02Z","title":"Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\\alpha$ Surface Brightness Ratio","version":1},"reference_index":248,"source":"arxiv_source","source_observed_at":"2026-06-27T21:13:45.849333Z"},"links":{"cited_paper":"/paper/2204.05316","citing_paper":"/paper/2606.07741"},"observation_digest":"sha256:bfad31969e75021fe312eb458b9602082bbd45b6dc50893b88960c69f3ecc733","observation_id":"0697fc40-373a-4abf-bfb1-4cf998d9f014","resolution":{"observed_at":"2026-07-02T19:57:19.633191Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2204.05316/citation-record","integrity":"/paper/2204.05316/integrity","json":"/paper/2204.05316/citation-record.json","paper":"/paper/2204.05316"},"outbound":[],"paper":{"arxiv_id":"2204.05316","last_updated":"2022-12-14T00:39:55Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T12:59:16.136198Z","submitted_at":"2022-04-11T18:00:00Z","title":"Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2204.05316."}