{"as_of":"2026-07-16T10:33:00Z","canonical_paper_id":"T5HLRYWS","canonical_url":"https://pith.science/paper/T5HLRYWS/integrity","context_digest":"sha256:a0e1b2deb0ed613d778697d58f0ee2869de5a800556b4b797e81dbc767b323a4","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/1903.02332","bundle_json":"/pith/T5HLRYWSLOHLEW7T757TS4PTIB/bundle.json","citation_record":"/paper/T5HLRYWS/citation-record","evidence":"/evidence","html":"/paper/T5HLRYWS/integrity","integrity_json":"/paper/T5HLRYWS/integrity.json","json":"/paper/T5HLRYWS/integrity.json","legacy_integrity_json":"/pith/T5HLRYWS/integrity.json","paper":"/paper/T5HLRYWS","reference_changes":"/flags?citing=T5HLRYWS"},"paper":{"arxiv_id":"1903.02332","latest_version":2,"primary_cat":"astro-ph.EP","title":"A high binary fraction for the most massive close-in giant planets and brown dwarf desert members"},"pith_number":"pith:2019:T5HLRYWSLOHLEW7T757TS4PTIB","pith_short":"T5HLRYWSLOHLEW7T757TS4PTIB","record":{"arxiv_id":"1903.02332","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1903.02332. 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"}