{"as_of":"2026-07-22T05:57:00Z","canonical_paper_id":"PYM5JVYZ","canonical_url":"https://pith.science/paper/PYM5JVYZ/integrity","context_digest":"sha256:7f66691a119e79cbaf342b5da0b52e400f30b8b9fb6959fc672fdc7d3dd48b69","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/1711.03161","bundle_json":"/pith/PYM5JVYZDPLGU3SC7WRT6VX4Z4/bundle.json","citation_record":"/paper/PYM5JVYZ/citation-record","evidence":"/evidence","html":"/paper/PYM5JVYZ/integrity","integrity_json":"/paper/PYM5JVYZ/integrity.json","json":"/paper/PYM5JVYZ/integrity.json","legacy_integrity_json":"/pith/PYM5JVYZ/integrity.json","paper":"/paper/PYM5JVYZ","reference_changes":"/flags?citing=PYM5JVYZ"},"paper":{"arxiv_id":"1711.03161","latest_version":2,"primary_cat":"astro-ph.GA","title":"Statistical properties of galactic CMB foregrounds: dust and synchrotron"},"pith_number":"pith:2017:PYM5JVYZDPLGU3SC7WRT6VX4Z4","pith_short":"PYM5JVYZDPLGU3SC7WRT6VX4Z4","record":{"arxiv_id":"1711.03161","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1711.03161. 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"}