{"as_of":"2026-07-16T11:15:00Z","canonical_paper_id":"2005.01726","canonical_url":"https://pith.science/paper/2005.01726/integrity","context_digest":"sha256:516086d67928ad503f6c41ef995493e5a73c68eb55a0cdd143d909b3bf70866e","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/2005.01726","bundle_json":"/pith/TTZ4H5ZU7QR7WU5ED275O34WNL/bundle.json","citation_record":"/paper/2005.01726/citation-record","evidence":"/evidence","html":"/paper/2005.01726/integrity","integrity_json":"/paper/2005.01726/integrity.json","json":"/paper/2005.01726/integrity.json","legacy_integrity_json":"/pith/2005.01726/integrity.json","paper":"/paper/2005.01726","reference_changes":"/flags?citing=2005.01726"},"paper":{"arxiv_id":"2005.01726","latest_version":2,"primary_cat":"astro-ph.HE","title":"Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations"},"pith_number":"pith:2020:TTZ4H5ZU7QR7WU5ED275O34WNL","pith_short":"TTZ4H5ZU7QR7WU5ED275O34WNL","record":{"arxiv_id":"2005.01726","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:2005.01726. 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"}