{"as_of":"2026-08-11T05:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:74e3d33f24616e8d648d3f6f4037adefe33b1ae2c2406dae28d9fe97252af0c2","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":"2026-08-10T06:31:04.303077+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":"2026-08-01T17:53:58.977077Z","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":"1404.2004","last_updated":"2015-02-01T15:06:16Z","snapshot_observed_at":"2026-08-03T04:42:55.685666Z","submitted_at":"2014-04-08T03:59:21Z","title":"Towards Characterization of the Type IIP Supernova Progenitor Population: a Statistical Sample of Light Curves from Pan-STARRS1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.2004","snapshot_observed_at":"2026-08-01T17:53:58.977077Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.17488","last_updated":"2026-07-20T02:24:30Z","snapshot_observed_at":"2026-08-06T02:38:55.369342Z","submitted_at":"2026-07-20T02:24:30Z","title":"Surrogate models for type II supernovae: Probing low-energy explosions and interaction-free regimes","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T17:53:58.977077Z"},"links":{"cited_paper":"/paper/1404.2004","citing_paper":"/paper/2607.17488"},"observation_digest":"sha256:f00e860ea5f2d7689463d26f27e86c6dfd3904ed84d8ff1b79df43e0026733a9","observation_id":"fda0e59f-a8fe-4382-8801-bdb2bcd78731","resolution":{"observed_at":"2026-08-01T17:53:58.977077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.2004","last_updated":"2015-02-01T15:06:16Z","snapshot_observed_at":"2026-08-03T04:42:55.685666Z","submitted_at":"2014-04-08T03:59:21Z","title":"Towards Characterization of the Type IIP Supernova Progenitor Population: a Statistical Sample of Light Curves from Pan-STARRS1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.2004","snapshot_observed_at":"2026-08-01T02:50:48.301194Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.25323","last_updated":"2026-07-28T06:14:24Z","snapshot_observed_at":"2026-08-06T21:16:56.879191Z","submitted_at":"2026-07-28T06:14:24Z","title":"SN 2022xus: bridging the gap between Type IIP and IIL supernovae","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-01T02:50:48.301194Z"},"links":{"cited_paper":"/paper/1404.2004","citing_paper":"/paper/2607.25323"},"observation_digest":"sha256:eef912585a8230b3833b7755d5ee011fe9ef189cbcdd754d29f89dcd87919c7f","observation_id":"d2d51fc4-544c-4b84-a259-53e3b1befcee","resolution":{"observed_at":"2026-08-01T02:50:48.301194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1404.2004/citation-record","integrity":"/paper/1404.2004/integrity","json":"/paper/1404.2004/citation-record.json","paper":"/paper/1404.2004"},"outbound":[],"paper":{"arxiv_id":"1404.2004","last_updated":"2015-02-01T15:06:16Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-03T04:42:55.685666Z","submitted_at":"2014-04-08T03:59:21Z","title":"Towards Characterization of the Type IIP Supernova Progenitor Population: a Statistical Sample of Light Curves from Pan-STARRS1"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1404.2004."}