{"as_of":"2026-07-14T10:07:00Z","canonical_paper_id":"2012.13060","canonical_url":"https://pith.science/paper/2012.13060/integrity","context_digest":"sha256:a96eadd6b5cb9b3f1f90c854ceefdd3ca5c9079f3da3d3969da562469c5b7d43","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/2012.13060","bundle_json":"/pith/QIVS6OW7TYWT3PF5EU5QGKGBH4/bundle.json","citation_record":"/paper/2012.13060/citation-record","evidence":"/evidence","html":"/paper/2012.13060/integrity","integrity_json":"/paper/2012.13060/integrity.json","json":"/paper/2012.13060/integrity.json","legacy_integrity_json":"/pith/2012.13060/integrity.json","paper":"/paper/2012.13060","reference_changes":"/flags?citing=2012.13060"},"paper":{"arxiv_id":"2012.13060","latest_version":1,"primary_cat":"astro-ph.GA","title":"Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network"},"pith_number":"pith:2020:QIVS6OW7TYWT3PF5EU5QGKGBH4","pith_short":"QIVS6OW7TYWT3PF5EU5QGKGBH4","record":{"arxiv_id":"2012.13060","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:2012.13060. 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"}