{"as_of":"2026-08-21T03:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5ba7bbaacc13086c520c2996a56b8cc7b77ef272f39d33abdb4a8a94b126a30a","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":"2026-08-20T06:33:59.587034+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":"2026-07-11T04:19:29.170180Z","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":"2026-07-11T04:27:47.855979Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2311.03120","last_updated":"2023-11-07T08:36:58Z","snapshot_observed_at":"2026-08-21T00:10:20.484162Z","submitted_at":"2023-11-06T14:15:00Z","title":"Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study","version":2},"cited_work":{"arxiv_id":"2311.03120","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.03120","snapshot_observed_at":"2026-07-11T04:27:47.855979Z","title":"Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study","venue":"astro-ph.SR","work_id":"1059e385-8e36-4982-a0f0-a13eb5f7e4ad","year":2023},"citing_paper":{"arxiv_id":"2607.05651","last_updated":"2026-07-06T21:31:54Z","snapshot_observed_at":"2026-07-11T04:19:17.632856Z","submitted_at":"2026-07-06T21:31:54Z","title":"Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-07-11T04:19:29.170180Z"},"links":{"cited_paper":"/paper/2311.03120","citing_paper":"/paper/2607.05651"},"observation_digest":"sha256:7ea1e86032cd59326c87f94373aef999e94d30e76f7e02f701cc757e92941b59","observation_id":"7ef6f90e-31ef-4ab3-862d-47e76d4a0fcd","resolution":{"observed_at":"2026-07-11T04:27:47.860663Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2311.03120/citation-record","integrity":"/paper/2311.03120/integrity","json":"/paper/2311.03120/citation-record.json","paper":"/paper/2311.03120"},"outbound":[],"paper":{"arxiv_id":"2311.03120","last_updated":"2023-11-07T08:36:58Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-21T00:10:20.484162Z","submitted_at":"2023-11-06T14:15:00Z","title":"Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2311.03120."}