{"as_of":"2026-08-15T12:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7f795ef0c385eaf6cd92cdec3074fb7c49642c7281f1f71710b84ce9acce82d3","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":"2026-08-14T10:38:08.690080Z","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":"2026-08-14T10:38:08.841184Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1804.10182","last_updated":"2018-04-26T17:33:47Z","snapshot_observed_at":"2026-08-15T10:16:07.314041Z","submitted_at":"2018-04-26T17:33:47Z","title":"Born-Infeld magnetars: larger than classical toroidal magnetic fields and implications for gravitational-wave astronomy","version":1},"cited_work":{"arxiv_id":"1804.10182","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.10182","snapshot_observed_at":"2026-08-14T10:38:08.841184Z","title":"Born-Infeld magnetars: larger than classical toroidal magnetic fields and implications for gravitational-wave astronomy","venue":"astro-ph.SR","work_id":"58ff1544-af21-402b-9af9-aca9bcc1e5bc","year":2018},"citing_paper":{"arxiv_id":"1908.11104","last_updated":"2020-05-11T15:57:21Z","snapshot_observed_at":"2026-08-15T10:15:58.934986Z","submitted_at":"2019-08-29T08:48:53Z","title":"Black hole magnetospheres in the Born-Infeld theory","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T10:38:08.690080Z"},"links":{"cited_paper":"/paper/1804.10182","citing_paper":"/paper/1908.11104"},"observation_digest":"sha256:a985d8bc88765ca22cff3108f5d931bfd50c9ba8dd7e2a0fa43d04f8325bcf79","observation_id":"40f80ea7-8ee4-4c8d-9b57-dae347fb4749","resolution":{"observed_at":"2026-08-14T10:38:08.845421Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1804.10182/citation-record","integrity":"/paper/1804.10182/integrity","json":"/paper/1804.10182/citation-record.json","paper":"/paper/1804.10182"},"outbound":[],"paper":{"arxiv_id":"1804.10182","last_updated":"2018-04-26T17:33:47Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-15T10:16:07.314041Z","submitted_at":"2018-04-26T17:33:47Z","title":"Born-Infeld magnetars: larger than classical toroidal magnetic fields and implications for gravitational-wave astronomy"},"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:1804.10182."}