{"as_of":"2026-08-13T19:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8dd55e14763a93a3c3c04b75a4c3473accb451806b6db820686bc968df912fb0","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":"2026-08-13T06:32:02.005865+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":"2026-08-12T12:06:52.894970Z","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":"2026-08-12T12:16:16.734455Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1906.04983","last_updated":"2019-06-12T07:47:06Z","snapshot_observed_at":"2026-07-06T07:59:46.057137Z","submitted_at":"2019-06-12T07:47:06Z","title":"Multiple Stellar Populations in NGC 2808: a Case Study for Cluster Analysis","version":1},"cited_work":{"arxiv_id":"1906.04983","doi":"10.48550/arxiv.1906.04983","metadata_source":"pith","pith_arxiv_id":"1906.04983","snapshot_observed_at":"2026-08-12T12:16:16.734455Z","title":"Multiple Stellar Populations in NGC 2808: a Case Study for Cluster Analysis","venue":"astro-ph.SR","work_id":"6247633d-b0a2-4330-abe0-253e272dad23","year":2019},"citing_paper":{"arxiv_id":"2411.17562","last_updated":"2024-11-26T16:24:59Z","snapshot_observed_at":"2026-08-12T11:56:45.132778Z","submitted_at":"2024-11-26T16:24:59Z","title":"Chemically Self-Consistent Modeling of the Globular Cluster NGC 2808 and its Effects on the Inferred Helium Abundance of Multiple Stellar Populations","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T12:06:52.894970Z"},"links":{"cited_paper":"/paper/1906.04983","citing_paper":"/paper/2411.17562"},"observation_digest":"sha256:93f16aa13fcbaf65964e55da42e3a5f11866479cb911a9fd095fc737bb964328","observation_id":"1af69874-de27-412d-9615-eeec45ecabc5","resolution":{"observed_at":"2026-08-12T12:06:53.075151Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1906.04983/citation-record","integrity":"/paper/1906.04983/integrity","json":"/paper/1906.04983/citation-record.json","paper":"/paper/1906.04983"},"outbound":[],"paper":{"arxiv_id":"1906.04983","last_updated":"2019-06-12T07:47:06Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T07:59:46.057137Z","submitted_at":"2019-06-12T07:47:06Z","title":"Multiple Stellar Populations in NGC 2808: a Case Study for Cluster Analysis"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1906.04983."}