{"as_of":"2026-08-12T16:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:69e02b4d3483a11b57f64329026527cf13126f21b5b7dde50e69c276f9364f49","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":"2026-08-12T06:34:41.77262+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":"2026-08-11T04:27:08.382393Z","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":"2026-08-10T21:46:30.823918Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2110.00018","last_updated":"2022-02-24T10:44:30Z","snapshot_observed_at":"2026-07-06T11:53:13.361514Z","submitted_at":"2021-09-30T18:00:02Z","title":"Measuring the Milky Way mass distribution in the presence of the LMC","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.00018","snapshot_observed_at":"2026-08-11T04:27:08.382393Z","title":"Correa Magnus, E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.18880","last_updated":"2025-07-28T13:23:47Z","snapshot_observed_at":"2026-08-11T04:19:46.498648Z","submitted_at":"2024-12-25T11:39:21Z","title":"Variable gravitational potential of Milky Way analogues in HESTIA suite","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T04:27:08.382393Z"},"links":{"cited_paper":"/paper/2110.00018","citing_paper":"/paper/2412.18880"},"observation_digest":"sha256:0d3ca508621890e610df1f7be5e012d9f4f2969ab04b98e7aeb5c9cb2bf7069b","observation_id":"538a5971-274b-494c-976f-2cc7c19aca98","resolution":{"observed_at":"2026-08-11T04:27:08.382393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.00018","last_updated":"2022-02-24T10:44:30Z","snapshot_observed_at":"2026-07-06T11:53:13.361514Z","submitted_at":"2021-09-30T18:00:02Z","title":"Measuring the Milky Way mass distribution in the presence of the LMC","version":2},"cited_work":{"arxiv_id":"2110.00018","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.00018","snapshot_observed_at":"2026-08-10T21:46:30.823918Z","title":"Measuring the Milky Way mass distribution in the presence of the LMC","venue":"astro-ph.GA","work_id":"bfd97dbc-0d1c-447c-8821-f441e3963a2b","year":2021},"citing_paper":{"arxiv_id":"2501.04075","last_updated":"2025-02-14T18:10:55Z","snapshot_observed_at":"2026-08-10T21:39:34.398532Z","submitted_at":"2025-01-07T19:00:00Z","title":"Milky Way dynamics in light of Gaia","version":2},"reference_index":2630,"source":"pdf_text","source_observed_at":"2026-08-10T21:46:29.989728Z"},"links":{"cited_paper":"/paper/2110.00018","citing_paper":"/paper/2501.04075"},"observation_digest":"sha256:de3a6e23e66279ab715084d9a6e72598f43ea430daface87679b5fa100e3ac16","observation_id":"60cdb33a-afde-45a4-9f31-fb1113f51dc9","resolution":{"observed_at":"2026-08-10T21:46:30.828591Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2110.00018/citation-record","integrity":"/paper/2110.00018/integrity","json":"/paper/2110.00018/citation-record.json","paper":"/paper/2110.00018"},"outbound":[],"paper":{"arxiv_id":"2110.00018","last_updated":"2022-02-24T10:44:30Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T11:53:13.361514Z","submitted_at":"2021-09-30T18:00:02Z","title":"Measuring the Milky Way mass distribution in the presence of the LMC"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2110.00018."}