{"as_of":"2026-08-22T19:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a2cdd2942878217e82e81f5c1ba6437723aeb48d424119f51dc663e2019e75d7","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T02:56:01.692740Z","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":"2026-07-01T05:15:24.810821Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1802.02824","last_updated":"2018-02-08T12:33:59Z","snapshot_observed_at":"2026-08-14T19:47:38.075575Z","submitted_at":"2018-02-08T12:33:59Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements","version":1},"cited_work":{"arxiv_id":"1802.02824","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.02824","snapshot_observed_at":"2026-07-01T05:15:24.810821Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements","venue":"astro-ph.GA","work_id":"390a2bc9-422b-4e8e-8a5c-8b2f779f1512","year":2018},"citing_paper":{"arxiv_id":"2605.23690","last_updated":"2026-05-22T14:47:42Z","snapshot_observed_at":"2026-08-19T03:04:43.595373Z","submitted_at":"2026-05-22T14:47:42Z","title":"The s- and r- components of the proto-solar composition","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1802.02824","citing_paper":"/paper/2605.23690"},"observation_digest":"sha256:07c4268f1205d28a1ed041dd85fcc46cb2102b330d3b94299e4a2c400fa2f99a","observation_id":"2cd11c73-dd64-4287-9c58-3a1aba524014","resolution":{"observed_at":"2026-05-25T02:55:15.069533Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02824","last_updated":"2018-02-08T12:33:59Z","snapshot_observed_at":"2026-08-14T19:47:38.075575Z","submitted_at":"2018-02-08T12:33:59Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements","version":1},"cited_work":{"arxiv_id":"1802.02824","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.02824","snapshot_observed_at":"2026-07-01T05:15:24.810821Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements","venue":"astro-ph.GA","work_id":"390a2bc9-422b-4e8e-8a5c-8b2f779f1512","year":2018},"citing_paper":{"arxiv_id":"2606.31218","last_updated":"2026-06-30T06:55:29Z","snapshot_observed_at":"2026-08-18T14:13:27.184125Z","submitted_at":"2026-06-30T06:55:29Z","title":"The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1802.02824","citing_paper":"/paper/2606.31218"},"observation_digest":"sha256:f724d8165a59587dd62849525328e713abbab408443bed9291e9e0b794f117db","observation_id":"5a5ba308-0002-4c4b-84f7-3ba16565baeb","resolution":{"observed_at":"2026-07-01T05:15:24.813615Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02824","last_updated":"2018-02-08T12:33:59Z","snapshot_observed_at":"2026-08-14T19:47:38.075575Z","submitted_at":"2018-02-08T12:33:59Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.02824","snapshot_observed_at":"2026-08-02T02:56:01.692740Z","title":"The solar neighbourhood and the s-process elements","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14067","last_updated":"2026-07-15T17:36:52Z","snapshot_observed_at":"2026-08-16T11:34:00.317225Z","submitted_at":"2026-07-15T17:36:52Z","title":"Magnesium isotope ratios in Milky Way and dwarf galaxy stars","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-08-02T02:56:01.692740Z"},"links":{"cited_paper":"/paper/1802.02824","citing_paper":"/paper/2607.14067"},"observation_digest":"sha256:e17ceccc7f1ee457faf5968ac38a92e201cc7ebc54e5415099ebed6bda04a93d","observation_id":"e7c04820-3c92-4538-9fbe-ae51a6eed2a9","resolution":{"observed_at":"2026-08-02T02:56:01.692740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1802.02824/citation-record","integrity":"/paper/1802.02824/integrity","json":"/paper/1802.02824/citation-record.json","paper":"/paper/1802.02824"},"outbound":[],"paper":{"arxiv_id":"1802.02824","last_updated":"2018-02-08T12:33:59Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T19:47:38.075575Z","submitted_at":"2018-02-08T12:33:59Z","title":"Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1802.02824."}