{"as_of":"2026-08-19T10:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e1cbaddfa035c6fa0efeda437ea32005a8a68123fb188e748871798b9f8713e2","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":"2026-08-19T06:32:44.657259+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":"2026-08-03T21:28:49.225891Z","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":"1204.2644","last_updated":"2012-04-12T07:43:05Z","snapshot_observed_at":"2026-08-15T04:13:18.645540Z","submitted_at":"2012-04-12T07:43:05Z","title":"Optimization of relativistic mean field model for finite nuclei to neutron star matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.2644","snapshot_observed_at":"2026-08-03T21:28:49.225891Z","title":"Optimiza tion of relativistic mean ﬁeld model for ﬁnite nuclei to neutron star matter,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.15385","last_updated":"2026-06-18T01:18:02Z","snapshot_observed_at":"2026-08-19T09:34:52.397536Z","submitted_at":"2025-11-19T12:26:56Z","title":"A relativistic mechanism for the enhanced isovector spin-orbit interaction suggested by parity-violating electron scattering experiments","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-03T21:28:49.225891Z"},"links":{"cited_paper":"/paper/1204.2644","citing_paper":"/paper/2511.15385"},"observation_digest":"sha256:75957f5a5d9d16c12da9b38beab5b84794f75ae2ff4f19c18b5da60c8be2d067","observation_id":"6ebf2233-9d6f-4a95-9a65-bae1fb5554e5","resolution":{"observed_at":"2026-08-03T21:28:49.225891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1204.2644/citation-record","integrity":"/paper/1204.2644/integrity","json":"/paper/1204.2644/citation-record.json","paper":"/paper/1204.2644"},"outbound":[],"paper":{"arxiv_id":"1204.2644","last_updated":"2012-04-12T07:43:05Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-15T04:13:18.645540Z","submitted_at":"2012-04-12T07:43:05Z","title":"Optimization of relativistic mean field model for finite nuclei to neutron star matter"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1204.2644."}