{"as_of":"2026-07-17T17:31:00Z","canonical_paper_id":"6IZLU3KW","canonical_url":"https://pith.science/paper/6IZLU3KW/integrity","context_digest":"sha256:76d69cb356155693d513b7eb80aee3a285d5265f4b9ddc6f54536467aa247b74","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/1207.5564","bundle_json":"/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/bundle.json","citation_record":"/paper/6IZLU3KW/citation-record","evidence":"/evidence","html":"/paper/6IZLU3KW/integrity","integrity_json":"/paper/6IZLU3KW/integrity.json","json":"/paper/6IZLU3KW/integrity.json","legacy_integrity_json":"/pith/6IZLU3KW/integrity.json","paper":"/paper/6IZLU3KW","reference_changes":"/flags?citing=6IZLU3KW"},"paper":{"arxiv_id":"1207.5564","latest_version":1,"primary_cat":"astro-ph.CO","title":"FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1"},"pith_number":"pith:2012:6IZLU3KW5SLYFQW6BN5R2Z2XEF","pith_short":"6IZLU3KW5SLYFQW6BN5R2Z2XEF","record":{"arxiv_id":"1207.5564","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1207.5564. 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"}