{"as_of":"2026-08-16T12:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fb928321bff96cedecd3820908cb73fe7a026630ad36f219fca34a45a4f1b380","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T22:03:07.594718Z","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":"2026-07-04T18:30:01.398354Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.08765","last_updated":"2025-03-11T18:00:00Z","snapshot_observed_at":"2026-08-07T17:12:08.515686Z","submitted_at":"2025-03-11T18:00:00Z","title":"Detection of magnetic fields in superclusters of galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.08765","snapshot_observed_at":"2026-08-15T22:03:07.594718Z","title":"V., O'Sullivan S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.08272","last_updated":"2025-05-13T06:36:19Z","snapshot_observed_at":"2026-08-15T21:56:42.413530Z","submitted_at":"2025-05-13T06:36:19Z","title":"The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description","version":1},"reference_index":172,"source":"arxiv_source","source_observed_at":"2026-08-15T22:03:07.594718Z"},"links":{"cited_paper":"/paper/2503.08765","citing_paper":"/paper/2505.08272"},"observation_digest":"sha256:25a19305ce150eb80d19ea21fc4e0606a3eeae3dd61a7e1d0c880d19d8a24ff0","observation_id":"2b1d0f53-0a28-4b73-aab2-6726ab3b0b9f","resolution":{"observed_at":"2026-08-15T22:03:07.594718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.08765","last_updated":"2025-03-11T18:00:00Z","snapshot_observed_at":"2026-08-07T17:12:08.515686Z","submitted_at":"2025-03-11T18:00:00Z","title":"Detection of magnetic fields in superclusters of galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.08765","snapshot_observed_at":"2026-08-07T14:35:20.255385Z","title":"Detection of magnetic fields in superclusters of galaxies","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18619","last_updated":"2025-05-24T10:03:09Z","snapshot_observed_at":"2026-08-07T21:18:38.197288Z","submitted_at":"2025-05-24T10:03:09Z","title":"Radio Observations as a Probe of Cosmic Web Magnetism","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T14:35:20.255385Z"},"links":{"cited_paper":"/paper/2503.08765","citing_paper":"/paper/2505.18619"},"observation_digest":"sha256:d534df5f994119c6caa032bdb2409c055cf700d5ea63acce4bbfdcb72725ba64","observation_id":"55ef3abb-8b76-446a-bb6c-eb1f6757cfbb","resolution":{"observed_at":"2026-08-07T14:35:20.255385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.08765","last_updated":"2025-03-11T18:00:00Z","snapshot_observed_at":"2026-08-07T17:12:08.515686Z","submitted_at":"2025-03-11T18:00:00Z","title":"Detection of magnetic fields in superclusters of galaxies","version":1},"cited_work":{"arxiv_id":"2503.08765","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.08765","snapshot_observed_at":"2026-07-04T18:30:01.398354Z","title":null,"venue":null,"work_id":"ff7a794a-9939-47b9-ad46-53ca5a3df65e","year":2025},"citing_paper":{"arxiv_id":"2606.25096","last_updated":"2026-06-23T19:01:14Z","snapshot_observed_at":"2026-08-06T12:39:57.106113Z","submitted_at":"2026-06-23T19:01:14Z","title":"An SKA-Low RM Grid for constraining the origin of cosmic magnetism","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-06-25T22:50:34.179828Z"},"links":{"cited_paper":"/paper/2503.08765","citing_paper":"/paper/2606.25096"},"observation_digest":"sha256:5635ba2d78928149e5d790b80e70f55a31ad3b0cbbbac3b6c3e5a9e1f1c1691f","observation_id":"4655d400-4a35-4a4a-a936-db0df5ad0325","resolution":{"observed_at":"2026-07-04T18:30:01.399864Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2503.08765/citation-record","integrity":"/paper/2503.08765/integrity","json":"/paper/2503.08765/citation-record.json","paper":"/paper/2503.08765"},"outbound":[],"paper":{"arxiv_id":"2503.08765","last_updated":"2025-03-11T18:00:00Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T17:12:08.515686Z","submitted_at":"2025-03-11T18:00:00Z","title":"Detection of magnetic fields in superclusters of galaxies"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2503.08765."}