{"as_of":"2026-08-05T20:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bffbcb714136bdcf5fc8f813e4f5cd926bc1465296b1223768ac29d67adb538a","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":"2026-08-05T06:32:48.257954+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":"2026-05-08T16:19:05.133108Z","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":"2026-05-11T18:16:12.580113Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1506.00005","last_updated":"2015-09-01T14:26:50Z","snapshot_observed_at":"2026-07-06T04:19:22.444137Z","submitted_at":"2015-05-29T20:00:40Z","title":"The large-scale properties of simulated cosmological magnetic fields","version":2},"cited_work":{"arxiv_id":"1506.00005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1506.00005","snapshot_observed_at":"2026-07-04T20:35:38.621711Z","title":"Marinacci, M","venue":null,"work_id":"69e09eb2-20e0-4b73-afb0-5f9eb60a6637","year":2015},"citing_paper":{"arxiv_id":"2605.05323","last_updated":"2026-05-06T18:00:44Z","snapshot_observed_at":"2026-08-02T14:56:42.851134Z","submitted_at":"2026-05-06T18:00:44Z","title":"Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-08T16:19:05.133108Z"},"links":{"cited_paper":"/paper/1506.00005","citing_paper":"/paper/2605.05323"},"observation_digest":"sha256:218df5a5d48652178bfa4da6fd8a3e913fb6bd6d079a3cd27c6742456d14a4e3","observation_id":"aa5fc8fa-f072-4937-a20c-c2ac15a71ab6","resolution":{"observed_at":"2026-07-04T20:35:38.621711Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1506.00005/citation-record","integrity":"/paper/1506.00005/integrity","json":"/paper/1506.00005/citation-record.json","paper":"/paper/1506.00005"},"outbound":[],"paper":{"arxiv_id":"1506.00005","last_updated":"2015-09-01T14:26:50Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T04:19:22.444137Z","submitted_at":"2015-05-29T20:00:40Z","title":"The large-scale properties of simulated cosmological magnetic 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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1506.00005."}