{"as_of":"2026-08-06T11:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fa9c89b44f08b6d0f260b9c943d0b055c49cd44597243497c7d7fc098092ed7b","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":"2026-08-06T06:34:29.942622+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":"2026-08-01T22:01:34.468748Z","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":"2504.18717","last_updated":"2025-04-25T22:07:12Z","snapshot_observed_at":"2026-07-06T21:15:02.308553Z","submitted_at":"2025-04-25T22:07:12Z","title":"exoALMA. X. channel maps reveal complex $^{12}$CO abundance distributions and a variety of kinematic structures with evidence for embedded planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.18717","snapshot_observed_at":"2026-08-01T22:01:34.468748Z","title":null,"venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.15923","last_updated":"2026-07-17T13:05:21Z","snapshot_observed_at":"2026-08-06T08:57:33.112967Z","submitted_at":"2026-07-17T13:05:21Z","title":"Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals","version":1},"reference_index":183,"source":"arxiv_source","source_observed_at":"2026-08-01T22:01:34.468748Z"},"links":{"cited_paper":"/paper/2504.18717","citing_paper":"/paper/2607.15923"},"observation_digest":"sha256:89b06668a2d927f6626dc827370042bcead21fdbcf4879b9697a0772e1257b8b","observation_id":"811288a2-da06-4801-8238-4ab43b0bdd8a","resolution":{"observed_at":"2026-08-01T22:01:34.468748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2504.18717/citation-record","integrity":"/paper/2504.18717/integrity","json":"/paper/2504.18717/citation-record.json","paper":"/paper/2504.18717"},"outbound":[],"paper":{"arxiv_id":"2504.18717","last_updated":"2025-04-25T22:07:12Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-07-06T21:15:02.308553Z","submitted_at":"2025-04-25T22:07:12Z","title":"exoALMA. X. channel maps reveal complex $^{12}$CO abundance distributions and a variety of kinematic structures with evidence for embedded planets"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2504.18717."}