{"as_of":"2026-08-11T06:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f50e56fbe9523dd0db8d7b1661bbbc260e0dae0038ee3ef13ab695f003147318","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":"2026-08-11T06:34:44.6726+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":"2026-08-01T19:35:40.077238Z","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":"2305.02253","last_updated":"2023-05-03T16:38:14Z","snapshot_observed_at":"2026-08-04T04:24:01.211145Z","submitted_at":"2023-05-03T16:38:14Z","title":"Observationally guided models for the solar dynamo and the role of the surface field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02253","snapshot_observed_at":"2026-08-01T19:35:40.077238Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.16939","last_updated":"2026-07-18T19:22:40Z","snapshot_observed_at":"2026-08-06T22:55:35.862130Z","submitted_at":"2026-07-18T19:22:40Z","title":"Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-01T19:35:40.077238Z"},"links":{"cited_paper":"/paper/2305.02253","citing_paper":"/paper/2607.16939"},"observation_digest":"sha256:924049b1554f07b1a42f0905bd21c205ccb01cc0f30969e7d7042dfd3aede719","observation_id":"51c02518-3514-48e2-8300-1f159c07cb24","resolution":{"observed_at":"2026-08-01T19:35:40.077238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.02253/citation-record","integrity":"/paper/2305.02253/integrity","json":"/paper/2305.02253/citation-record.json","paper":"/paper/2305.02253"},"outbound":[],"paper":{"arxiv_id":"2305.02253","last_updated":"2023-05-03T16:38:14Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-04T04:24:01.211145Z","submitted_at":"2023-05-03T16:38:14Z","title":"Observationally guided models for the solar dynamo and the role of the surface field"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2305.02253."}