{"as_of":"2026-08-11T08:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b56bc8e9e17f9dec38a1720151648fc376eb9d2c5bd4de63b58ad92cf8d3af92","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":"2026-08-01T19:35:41.193025Z","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":"1606.07375","last_updated":"2017-01-12T20:45:02Z","snapshot_observed_at":"2026-07-06T05:01:05.782622Z","submitted_at":"2016-06-23T16:59:26Z","title":"A coupled $2\\times2$D Babcock-Leighton solar dynamo model. II. Reference dynamo solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07375","snapshot_observed_at":"2026-08-01T19:35:41.193025Z","title":null,"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":49,"source":"arxiv_source","source_observed_at":"2026-08-01T19:35:41.193025Z"},"links":{"cited_paper":"/paper/1606.07375","citing_paper":"/paper/2607.16939"},"observation_digest":"sha256:0605947cb3582c321cb1c83e6d93dd2d777960acca0671976da82b84c124f1b7","observation_id":"c0a5321d-0ca4-4ca6-b48e-a2d4c32de452","resolution":{"observed_at":"2026-08-01T19:35:41.193025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1606.07375/citation-record","integrity":"/paper/1606.07375/integrity","json":"/paper/1606.07375/citation-record.json","paper":"/paper/1606.07375"},"outbound":[],"paper":{"arxiv_id":"1606.07375","last_updated":"2017-01-12T20:45:02Z","latest_version":3,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T05:01:05.782622Z","submitted_at":"2016-06-23T16:59:26Z","title":"A coupled $2\\times2$D Babcock-Leighton solar dynamo model. II. Reference dynamo solutions"},"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:1606.07375."}