{"as_of":"2026-08-09T21:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:99a27d1b681da781a6d11fc6dc8897c176aa784d7103cc79aa472797bcaeeaa7","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":"2026-08-09T06:31:02.800959+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":"2026-08-07T21:05:50.513039Z","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":"2410.23167","last_updated":"2025-01-28T13:51:20Z","snapshot_observed_at":"2026-08-08T12:23:36.387376Z","submitted_at":"2024-10-30T16:18:53Z","title":"BPASS stellar evolution models incorporating $\\alpha$-enhanced composition -- I. Single star models from 0.1 to 316 M$_\\odot$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.23167","snapshot_observed_at":"2026-08-07T21:05:50.513039Z","title":"M., Eldridge J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09579","last_updated":"2025-03-13T11:45:48Z","snapshot_observed_at":"2026-08-07T20:55:01.129066Z","submitted_at":"2025-02-13T18:36:16Z","title":"Comparison of methods used to derive the Galactic star formation history from white dwarf samples","version":3},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-07T21:05:50.513039Z"},"links":{"cited_paper":"/paper/2410.23167","citing_paper":"/paper/2502.09579"},"observation_digest":"sha256:04da0df1a22c60add1614d0794cda7ee2ae0cb396737cfca0ca79f907279d60e","observation_id":"41fb0163-3c31-4426-9766-e57251484360","resolution":{"observed_at":"2026-08-07T21:05:50.513039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.23167","last_updated":"2025-01-28T13:51:20Z","snapshot_observed_at":"2026-08-08T12:23:36.387376Z","submitted_at":"2024-10-30T16:18:53Z","title":"BPASS stellar evolution models incorporating $\\alpha$-enhanced composition -- I. Single star models from 0.1 to 316 M$_\\odot$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.23167","snapshot_observed_at":"2026-08-02T00:50:15.023720Z","title":"Single star models from 0.1 to 316 M _","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14901","last_updated":"2026-07-16T12:17:52Z","snapshot_observed_at":"2026-08-08T00:49:11.157835Z","submitted_at":"2026-07-16T12:17:52Z","title":"The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-02T00:50:15.023720Z"},"links":{"cited_paper":"/paper/2410.23167","citing_paper":"/paper/2607.14901"},"observation_digest":"sha256:7db1c2869cb69d8f819f28f08d1468f5d10307bd2d25f9229c7e9e9bb6d2dba0","observation_id":"82fcb0a4-fe7c-42c9-86a2-2a91f147d040","resolution":{"observed_at":"2026-08-02T00:50:15.023720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.23167/citation-record","integrity":"/paper/2410.23167/integrity","json":"/paper/2410.23167/citation-record.json","paper":"/paper/2410.23167"},"outbound":[],"paper":{"arxiv_id":"2410.23167","last_updated":"2025-01-28T13:51:20Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-08T12:23:36.387376Z","submitted_at":"2024-10-30T16:18:53Z","title":"BPASS stellar evolution models incorporating $\\alpha$-enhanced composition -- I. Single star models from 0.1 to 316 M$_\\odot$"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.23167."}