{"as_of":"2026-07-15T06:00:00Z","canonical_paper_id":"M6YYPYTO","canonical_url":"https://pith.science/paper/M6YYPYTO/integrity","context_digest":"sha256:36352d688165705b3f2d292c246de45e5c6ccc2d94c083c55f7c7bc0c8e1051e","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/1011.3018","bundle_json":"/pith/M6YYPYTOG3UF3ZJ6P3MY5M55PA/bundle.json","citation_record":"/paper/M6YYPYTO/citation-record","evidence":"/evidence","html":"/paper/M6YYPYTO/integrity","integrity_json":"/paper/M6YYPYTO/integrity.json","json":"/paper/M6YYPYTO/integrity.json","legacy_integrity_json":"/pith/M6YYPYTO/integrity.json","paper":"/paper/M6YYPYTO","reference_changes":"/flags?citing=M6YYPYTO"},"paper":{"arxiv_id":"1011.3018","latest_version":3,"primary_cat":"astro-ph.CO","title":"HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion"},"pith_number":"pith:2010:M6YYPYTOG3UF3ZJ6P3MY5M55PA","pith_short":"M6YYPYTOG3UF3ZJ6P3MY5M55PA","record":{"arxiv_id":"1011.3018","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1011.3018. 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"}