{"as_of":"2026-08-13T09:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5bf7c1aab5d2839c7d2875db8025af95fd9a4c4acfafe84fdf6e94755a61adb9","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":"2026-08-13T06:32:02.005865+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":"2026-08-11T22:20:16.552102Z","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":"2026-08-11T22:20:16.693396Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.14419","last_updated":"2020-04-29T18:31:54Z","snapshot_observed_at":"2026-08-13T02:30:58.456677Z","submitted_at":"2020-04-29T18:31:54Z","title":"Type IIP Supernova Progenitors III: Blue to Red Supergiant Ratio in Low Metallicity Models with Convective Overshoot","version":1},"cited_work":{"arxiv_id":"2004.14419","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.14419","snapshot_observed_at":"2026-08-11T22:20:16.693396Z","title":"Type IIP Supernova Progenitors III: Blue to Red Supergiant Ratio in Low Metallicity Models with Convective Overshoot","venue":"astro-ph.SR","work_id":"469a0fd8-b684-40f7-9f37-fcd98caf5177","year":2020},"citing_paper":{"arxiv_id":"2412.03652","last_updated":"2025-04-04T23:19:34Z","snapshot_observed_at":"2026-08-13T04:34:03.313100Z","submitted_at":"2024-12-04T19:00:01Z","title":"Blue Loops, Cepheids, and Forays into Axions","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T22:20:16.552102Z"},"links":{"cited_paper":"/paper/2004.14419","citing_paper":"/paper/2412.03652"},"observation_digest":"sha256:3a5bc16dcd134be80d89ec2d4f4c695da4bc052f96cdbb8342fc81b33159d3bf","observation_id":"cdddf355-f434-43ec-b2e5-ff0a917389ac","resolution":{"observed_at":"2026-08-11T22:20:16.698179Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2004.14419/citation-record","integrity":"/paper/2004.14419/integrity","json":"/paper/2004.14419/citation-record.json","paper":"/paper/2004.14419"},"outbound":[],"paper":{"arxiv_id":"2004.14419","last_updated":"2020-04-29T18:31:54Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-13T02:30:58.456677Z","submitted_at":"2020-04-29T18:31:54Z","title":"Type IIP Supernova Progenitors III: Blue to Red Supergiant Ratio in Low Metallicity Models with Convective Overshoot"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2004.14419."}