{"as_of":"2026-08-15T19:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:719bc8742a821bf4e294870a1603131b8238596b471e6388983364e44d07c05f","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":"2026-08-15T06:32:42.880941+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":"2026-08-03T15:48:51.451041Z","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":"2410.05388","last_updated":"2025-06-11T21:02:34Z","snapshot_observed_at":"2026-08-12T22:28:52.444753Z","submitted_at":"2024-10-07T18:00:08Z","title":"Generation of Large-scale Magnetic Fields Upstream of Gamma-Ray Burst Afterglow Shocks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05388","snapshot_observed_at":"2026-08-03T15:48:51.451041Z","title":"Generation of large-scale magnetic fields up- stream of gamma-ray burst afterglow shocks,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.15847","last_updated":"2026-07-16T18:13:20Z","snapshot_observed_at":"2026-08-10T10:46:59.686678Z","submitted_at":"2025-12-17T19:00:00Z","title":"Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T15:48:51.451041Z"},"links":{"cited_paper":"/paper/2410.05388","citing_paper":"/paper/2512.15847"},"observation_digest":"sha256:a12c864c1c5aed98350abc31d8fbad4709bf5431fcaa345ae1ab7beb6716877a","observation_id":"f324bd5a-f659-4e0e-85fd-fab24dada5a8","resolution":{"observed_at":"2026-08-03T15:48:51.451041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.05388/citation-record","integrity":"/paper/2410.05388/integrity","json":"/paper/2410.05388/citation-record.json","paper":"/paper/2410.05388"},"outbound":[],"paper":{"arxiv_id":"2410.05388","last_updated":"2025-06-11T21:02:34Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-12T22:28:52.444753Z","submitted_at":"2024-10-07T18:00:08Z","title":"Generation of Large-scale Magnetic Fields Upstream of Gamma-Ray Burst Afterglow Shocks"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2410.05388."}