{"as_of":"2026-07-20T09:58:00Z","canonical_paper_id":"U6HG545K","canonical_url":"https://pith.science/paper/U6HG545K/integrity","context_digest":"sha256:e985691b053bc865daa58662df07312fbcd1214e0d8f966cd8b58b80e3b0aef5","coverage_summary":[],"findings":[],"findings_empty_copy":"No checks are listed for this paper yet.","findings_observation_state":"no_listed_checks","links":{"arxiv":"https://arxiv.org/abs/1612.02805","bundle_json":"/pith/U6HG545KHFTTJZZYCSZMEOZD27/bundle.json","citation_record":"/paper/U6HG545K/citation-record","evidence":"/evidence","html":"/paper/U6HG545K/integrity","integrity_json":"/paper/U6HG545K/integrity.json","json":"/paper/U6HG545K/integrity.json","legacy_integrity_json":"/pith/U6HG545K/integrity.json","paper":"/paper/U6HG545K","reference_changes":"/flags?citing=U6HG545K"},"paper":{"arxiv_id":"1612.02805","latest_version":3,"primary_cat":"astro-ph.HE","title":"Exploring the efficacy and limitations of shock-cooling models: new analysis of Type II supernovae observed by the Kepler mission"},"pith_number":"pith:2016:U6HG545KHFTTJZZYCSZMEOZD27","pith_short":"U6HG545KHFTTJZZYCSZMEOZD27","record":{"arxiv_id":"1612.02805","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1612.02805. No listed check completed, so this record makes no findings claim.","counts":{"completed":0,"failed":0,"listed":0,"not_collected":0,"not_requested":0,"partial":0,"public_findings_from_completed":0,"skipped":0,"unavailable":0,"withheld":0},"coverage":[],"observed_at":null,"refusal":"This is a record of named checks, not a clean-status claim or a paper verdict.","schema":"pith.integrity.v1"},"schema":"pith.paper-integrity-record.v1","species":"LEDGER"}