{"as_of":"2026-07-16T16:58:00Z","canonical_paper_id":"2602.18340","canonical_url":"https://pith.science/paper/2602.18340/integrity","context_digest":"sha256:9696512d7fd97383c08b7620174bfb56aff4278bcb6959a53414cbd1173116e5","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/2602.18340","bundle_json":"","citation_record":"/paper/2602.18340/citation-record","evidence":"/evidence","html":"/paper/2602.18340/integrity","integrity_json":"/paper/2602.18340/integrity.json","json":"/paper/2602.18340/integrity.json","legacy_integrity_json":"/pith/2602.18340/integrity.json","paper":"/paper/2602.18340","reference_changes":"/flags?citing=2602.18340"},"paper":{"arxiv_id":"2602.18340","latest_version":2,"primary_cat":"astro-ph.SR","title":"A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks"},"pith_number":null,"pith_short":null,"record":{"arxiv_id":"2602.18340","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:2602.18340. 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"}