{"schema":"https://pith.science/schemas/pith-integrity/v1.json","pith_number":"2605.03500","arxiv_id":"2605.03500","integrity":{"available":true,"endpoint":"/pith/2605.03500/integrity.json","summary":{"critical":0,"advisory":1,"informational":0,"by_detector":{"doi_compliance":{"total":1,"critical":0,"advisory":1,"informational":0}}},"clean":false,"detectors_run":[{"name":"ai_meta_artifact","version":"1.0.0","status":"completed","ran_at":"2026-05-20T13:39:51.851164Z","findings_count":0},{"name":"doi_title_agreement","version":"1.0.0","status":"completed","ran_at":"2026-05-20T01:01:21.671066Z","findings_count":0},{"name":"doi_compliance","version":"1.0.0","status":"completed","ran_at":"2026-05-19T15:18:05.160073Z","findings_count":1}],"findings":[{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1051/0004-6361:2007826332) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1051/0004-6361:2007826332","detected_arxiv_id":null,"ref_index":7,"audited_at":"2026-05-19T15:18:05.160073Z"}],"snapshot_sha256":"74fdc3ce0ff2dbe0bf8c4012236257c05aa45207dee148247a22ab8ab6e6199e"},"events":[{"event_id":1829,"event_type":"pith.integrity.v1","payload_sha256":"ef5fc780cd83d72b7f86e266399d46fbb430cbe547709c48184f8688f5892576","signature_b64":"kYxWC2Z2H2hsHH1Mprt00Pq4EM9BaRYvjvjT3/dvoW5AXU4OMIcsUOLFThQUt5YstJhrTANJjgZy9zPjKw/VDw==","signing_key_id":"pith-v1-2026-05","created_at":"2026-05-19T15:22:10.225710+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1051/0004-6361:2007826332) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"Buat, V., Boissier, S., Burgarella, D., Takeuchi, T. T., Le Floc’h, E., Marcillac, D., Huang, J., Nagashima, M., & Enoki, M. (2008). Star formation history of galaxies from z = 0 to z = 0.7. A backward approach to the evolution of star-form","arxiv_id":"2605.03500","detector":"doi_compliance","evidence":{"ref_index":7,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"Buat, V., Boissier, S., Burgarella, D., Takeuchi, T. T., Le Floc’h, E., Marcillac, D., Huang, J., Nagashima, M., & Enoki, M. (2008). Star formation history of galaxies from z = 0 to z = 0.7. A backward approach to the evolution of star-form","reconstructed_doi":"10.1051/0004-6361:2007826332"},"severity":"advisory","ref_index":7,"audited_at":"2026-05-19T15:18:05.160073Z","event_type":"pith.integrity.v1","detected_doi":"10.1051/0004-6361:2007826332","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"4cfaf8937342b8b89fa2725d45ecd9461d0d14b40b6d315d7eac664264f68256","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null}}],"endpoint_self":"/pith/2605.03500/integrity.json","protocol_url":"https://pith.science/pith-integrity-protocol"}