{"as_of":"2026-08-17T15:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:def341421310d9b786bf362531d1ed787fe4f84db8dc20b7e0bd917d7a07fae3","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":"2026-08-17T06:30:58.91139+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":"2026-08-02T02:59:16.395453Z","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":"2101.02348","last_updated":"2021-01-07T03:19:06Z","snapshot_observed_at":"2026-08-16T18:53:49.253211Z","submitted_at":"2021-01-07T03:19:06Z","title":"Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.02348","snapshot_observed_at":"2026-08-02T02:58:16.014118Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14065","last_updated":"2026-07-15T17:36:36Z","snapshot_observed_at":"2026-08-15T20:59:18.314364Z","submitted_at":"2026-07-15T17:36:36Z","title":"The complex stellar system M 22: confirming abundance variations with high precision differential measurements","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-02T02:58:16.014118Z"},"links":{"cited_paper":"/paper/2101.02348","citing_paper":"/paper/2607.14065"},"observation_digest":"sha256:d837628b1579a84221e7681fb9d3f16b56484f99cf4afb5bcb430fcb6e5a9630","observation_id":"4e309697-cd59-4231-99af-4223635c819e","resolution":{"observed_at":"2026-08-02T02:58:16.014118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.02348","last_updated":"2021-01-07T03:19:06Z","snapshot_observed_at":"2026-08-16T18:53:49.253211Z","submitted_at":"2021-01-07T03:19:06Z","title":"Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.02348","snapshot_observed_at":"2026-08-02T02:59:16.395453Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.395453Z"},"links":{"cited_paper":"/paper/2101.02348","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:01462ec8b57cbe4d8ad939b959978a777e051d098500be7559f605ac82319922","observation_id":"4020ca52-f81f-444e-846d-7be623f8dca4","resolution":{"observed_at":"2026-08-02T02:59:16.395453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2101.02348/citation-record","integrity":"/paper/2101.02348/integrity","json":"/paper/2101.02348/citation-record.json","paper":"/paper/2101.02348"},"outbound":[],"paper":{"arxiv_id":"2101.02348","last_updated":"2021-01-07T03:19:06Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T18:53:49.253211Z","submitted_at":"2021-01-07T03:19:06Z","title":"Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2101.02348."}