{"as_of":"2026-08-19T03:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a0a588ec642b049b0ebc0b965038ee8d0ce7784d93113fa5845e15a6c120ef81","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":"2026-08-18T06:34:40.430872+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":"2026-08-10T13:20:41.710488Z","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":"1706.00939","last_updated":"2017-06-03T12:13:07Z","snapshot_observed_at":"2026-08-14T20:56:19.461743Z","submitted_at":"2017-06-03T12:13:07Z","title":"The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.00939","snapshot_observed_at":"2026-08-10T13:20:41.710488Z","title":"title The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-17T09:28:31.322424Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":199,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.710488Z"},"links":{"cited_paper":"/paper/1706.00939","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:4defa5a4b26a3988c6ea408e570749a7fbab53eeb40bbadcf44d558659cf374a","observation_id":"3d108b3d-80a7-4481-9af2-eb168c0e3d38","resolution":{"observed_at":"2026-08-10T13:20:41.710488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.00939","last_updated":"2017-06-03T12:13:07Z","snapshot_observed_at":"2026-08-14T20:56:19.461743Z","submitted_at":"2017-06-03T12:13:07Z","title":"The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.00939","snapshot_observed_at":"2026-08-03T19:35:04.047299Z","title":"Lamers, J.M.D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.23452","last_updated":"2026-07-05T17:17:05Z","snapshot_observed_at":"2026-08-17T09:37:10.938797Z","submitted_at":"2025-11-28T18:43:46Z","title":"From metallicity distributions to mutual information: A new perspective on stellar halo assembly","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T19:35:04.047299Z"},"links":{"cited_paper":"/paper/1706.00939","citing_paper":"/paper/2511.23452"},"observation_digest":"sha256:10b3b5df7f67eecb46b7f39563c65ba289a88e303fa4e772b6fead4038249b5b","observation_id":"b9090fe4-2afb-447e-a627-eb437af030e4","resolution":{"observed_at":"2026-08-03T19:35:04.047299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1706.00939/citation-record","integrity":"/paper/1706.00939/integrity","json":"/paper/1706.00939/citation-record.json","paper":"/paper/1706.00939"},"outbound":[],"paper":{"arxiv_id":"1706.00939","last_updated":"2017-06-03T12:13:07Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T20:56:19.461743Z","submitted_at":"2017-06-03T12:13:07Z","title":"The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1706.00939."}