{"as_of":"2026-07-18T21:22:00Z","canonical_paper_id":"1005.3852","canonical_url":"https://pith.science/paper/1005.3852/integrity","context_digest":"sha256:6f3b1eb5c116984c68d87b30c756e343f0763888d7cf2e0b47cd42893b2e515f","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/1005.3852","bundle_json":"/pith/5V4HJH2HQ2B2W4DO5RPJJQL6BW/bundle.json","citation_record":"/paper/1005.3852/citation-record","evidence":"/evidence","html":"/paper/1005.3852/integrity","integrity_json":"/paper/1005.3852/integrity.json","json":"/paper/1005.3852/integrity.json","legacy_integrity_json":"/pith/1005.3852/integrity.json","paper":"/paper/1005.3852","reference_changes":"/flags?citing=1005.3852"},"paper":{"arxiv_id":"1005.3852","latest_version":2,"primary_cat":"astro-ph.CO","title":"A Far-IR Characterization of 24 micron Selected Galaxies at 0<z<2.5 using Stacking at 70 microns and 160 microns in the COSMOS Field"},"pith_number":"pith:2010:5V4HJH2HQ2B2W4DO5RPJJQL6BW","pith_short":"5V4HJH2HQ2B2W4DO5RPJJQL6BW","record":{"arxiv_id":"1005.3852","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1005.3852. 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"}