{"as_of":"2026-07-20T12:36:00Z","canonical_paper_id":"2005.07188","canonical_url":"https://pith.science/paper/2005.07188/integrity","context_digest":"sha256:1381c4d76b6990d46a1fd2d2f07313577feb9a33df0e1fdd9138fbbc4ef2fb19","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/2005.07188","bundle_json":"/pith/FH6UCAGSP7V73UJ4OLY53TXJAY/bundle.json","citation_record":"/paper/2005.07188/citation-record","evidence":"/evidence","html":"/paper/2005.07188/integrity","integrity_json":"/paper/2005.07188/integrity.json","json":"/paper/2005.07188/integrity.json","legacy_integrity_json":"/pith/2005.07188/integrity.json","paper":"/paper/2005.07188","reference_changes":"/flags?citing=2005.07188"},"paper":{"arxiv_id":"2005.07188","latest_version":3,"primary_cat":"gr-qc","title":"Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?"},"pith_number":"pith:2020:FH6UCAGSP7V73UJ4OLY53TXJAY","pith_short":"FH6UCAGSP7V73UJ4OLY53TXJAY","record":{"arxiv_id":"2005.07188","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:2005.07188. 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"}