{"as_of":"2026-08-21T01:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e34fb103a210af12fc16fae306f56d8226ece5594810fe91c708125c041f5e94","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":"2026-08-20T06:33:59.587034+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":"2026-08-11T11:59:43.051437Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-11T12:16:16.480190Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.14596","last_updated":"2024-11-04T11:26:37Z","snapshot_observed_at":"2026-08-16T13:32:36.998661Z","submitted_at":"2024-07-19T18:00:02Z","title":"A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6","version":3},"cited_work":{"arxiv_id":"2407.14596","doi":"10.48550/arxiv.2407.14596","metadata_source":"pith","pith_arxiv_id":"2407.14596","snapshot_observed_at":"2026-08-11T12:16:16.480190Z","title":"A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6","venue":"astro-ph.GA","work_id":"09446a77-c4b5-4899-aab9-8186c873f78e","year":2024},"citing_paper":{"arxiv_id":"2412.14770","last_updated":"2024-12-19T11:54:16Z","snapshot_observed_at":"2026-08-14T00:00:43.827634Z","submitted_at":"2024-12-19T11:54:16Z","title":"Polarized Dust Emission in Arp220: Magnetic Fields in the Core of an Ultraluminous Infrared Galaxy","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-11T11:59:43.051437Z"},"links":{"cited_paper":"/paper/2407.14596","citing_paper":"/paper/2412.14770"},"observation_digest":"sha256:d2847958dd6e2f19e8be213c6d80e44528d4b43e0362ec01177f24e47b07d6e0","observation_id":"84a21e9b-dc4f-4cb2-abe1-bb3598ba6586","resolution":{"observed_at":"2026-08-11T11:59:43.512872Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14596","last_updated":"2024-11-04T11:26:37Z","snapshot_observed_at":"2026-08-16T13:32:36.998661Z","submitted_at":"2024-07-19T18:00:02Z","title":"A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14596","snapshot_observed_at":"2026-07-31T14:25:21.919253Z","title":"arXiv , author =:2407.14596 , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.24461","last_updated":"2026-07-27T14:01:57Z","snapshot_observed_at":"2026-08-13T14:42:26.431396Z","submitted_at":"2026-07-27T14:01:57Z","title":"Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-31T14:25:21.919253Z"},"links":{"cited_paper":"/paper/2407.14596","citing_paper":"/paper/2607.24461"},"observation_digest":"sha256:d57ae087288032040e699ba351f5b569da13ab53d5b2c049f776a55f3250321e","observation_id":"4b96dee4-a35f-41ca-9e30-a28d8ad1d1e6","resolution":{"observed_at":"2026-07-31T14:25:21.919253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.14596/citation-record","integrity":"/paper/2407.14596/integrity","json":"/paper/2407.14596/citation-record.json","paper":"/paper/2407.14596"},"outbound":[],"paper":{"arxiv_id":"2407.14596","last_updated":"2024-11-04T11:26:37Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T13:32:36.998661Z","submitted_at":"2024-07-19T18:00:02Z","title":"A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.14596."}