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A longer candidate (10.1088/1538-3873/ac1c5f) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1088/1538-3873/ac1c5f","detected_arxiv_id":null,"ref_index":51,"audited_at":"2026-08-02T02:39:38.231823Z"},{"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 (10.3847/1538-3881/aabc4f) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.3847/1538-3881/aabc4f","detected_arxiv_id":null,"ref_index":58,"audited_at":"2026-08-02T02:39:38.231823Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI is split by whitespace or line breaks in the printed bibliography. Reconstructed DOI 10.1146/annurev.astro.46.060407.145222 resolves to 'The Chemical Composition of the Sun'. A reader following the printed text alone cannot reach it.","detected_doi":"10.1146/annurev.astro.46.060407.145222","detected_arxiv_id":null,"ref_index":84,"audited_at":"2026-08-02T02:39:38.231823Z"}],"snapshot_sha256":"87ef9f0623ccab94b424fca90d8d4be6c5c92840ffa80a79f60507f2849880fe"},"events":[{"event_id":17072,"event_type":"pith.integrity.v1","payload_sha256":"a2e4ede68ce6e1d95d9e4e10f4ad6a361defb07cf031ae7369a543e9b5ab3a04","signature_b64":"pPij0dCmVd4j/felT6onTckrSKOATJpaCR4wHbs4EYFEnHY+GNAtWX7yPlT8A51oASGblqg+feopkGg279DfAw==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-02T02:43:30.476852+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1051/0004-6361/201833316) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"E. 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Reconstructed DOI 10.1126/science.aat5879 resolves to 'Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet'. A reader following the printed text alone cannot reach it.","snippet":"R. 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A longer candidate (10.1088/0004-637X/814/2/100) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"P. G. Judge, L. Kleint, A. Sainz Dalda, On Helium 1083 nm Line Polarization during the Impulsive Phase of an X1 Flare.Astrophys. 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Reconstructed DOI 10.1146/annurev.astro.46.060407.145222 resolves to 'The Chemical Composition of the Sun'. A reader following the printed text alone cannot reach it.","snippet":"M. Asplund, N. Grevesse, A. J. Sauval, P. Scott, The Chemical Composition of the Sun. 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A longer candidate (10.3847/1538-3881/aabc4f) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"Astropy Collaboration,et al., The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package.Astron. 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Reconstructed DOI 10.1093/mnras/sty290 resolves to 'Core-powered mass-loss and the radius distribution of small exoplanets'. A reader following the printed text alone cannot reach it.","snippet":"S. Ginzburg, H. E. Schlichting, R. Sari, Core-powered mass-loss and the radius distribution of small exoplanets.Mon. Not. R. Astron. 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