{"as_of":"2026-08-10T19:36:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4c18e4692046584f089ed743413505627d2372070cc4edd8d200c1210baed5e8","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T06:46:18.664746Z","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":"1606.02368","last_updated":"2016-06-08T01:21:41Z","snapshot_observed_at":"2026-07-06T04:59:09.337012Z","submitted_at":"2016-06-08T01:21:41Z","title":"Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02368","snapshot_observed_at":"2026-08-01T19:35:37.300832Z","title":"Solar Physics , 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":15,"source":"arxiv_source","source_observed_at":"2026-08-01T19:35:37.300832Z"},"links":{"cited_paper":"/paper/1606.02368","citing_paper":"/paper/2607.16939"},"observation_digest":"sha256:23da1f0f689df4f4f00d244718379fc9186d77928c135615a58b8d06ca161bf5","observation_id":"b0e04cb3-f5e7-4a4f-96ed-200ed2c2e5e1","resolution":{"observed_at":"2026-08-01T19:35:37.300832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02368","last_updated":"2016-06-08T01:21:41Z","snapshot_observed_at":"2026-07-06T04:59:09.337012Z","submitted_at":"2016-06-08T01:21:41Z","title":"Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02368","snapshot_observed_at":"2026-08-03T06:46:18.664746Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.664746Z"},"links":{"cited_paper":"/paper/1606.02368","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1c92bf9e7bc41864a14914ec6f4f2e78f8033db91d8072747ecedb1ff0d9894e","observation_id":"5b90e401-a6f4-4879-99e1-3fa7205666d9","resolution":{"observed_at":"2026-08-03T06:46:18.664746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1606.02368/citation-record","integrity":"/paper/1606.02368/integrity","json":"/paper/1606.02368/citation-record.json","paper":"/paper/1606.02368"},"outbound":[],"paper":{"arxiv_id":"1606.02368","last_updated":"2016-06-08T01:21:41Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T04:59:09.337012Z","submitted_at":"2016-06-08T01:21:41Z","title":"Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1606.02368."}