{"schema":"https://pith.science/schemas/pith-integrity/v1.json","pith_number":"2608.07951","arxiv_id":"2608.07951","integrity":{"available":true,"endpoint":"/pith/2608.07951/integrity.json","summary":{"critical":2,"advisory":3,"informational":0,"by_detector":{"doi_compliance":{"total":5,"critical":2,"advisory":3,"informational":0}}},"clean":false,"detectors_run":[{"name":"claim_evidence","version":"1.0.0","status":"completed","ran_at":"2026-08-12T06:28:08.143354Z","findings_count":0},{"name":"doi_title_agreement","version":"1.0.0","status":"completed","ran_at":"2026-08-12T01:08:45.903978Z","findings_count":0},{"name":"doi_compliance","version":"1.1.0","status":"completed","ran_at":"2026-08-12T00:58:24.590379Z","findings_count":5},{"name":"ai_meta_artifact","version":"1.0.0","status":"skipped","ran_at":"2026-08-11T05:08:44.530881Z","findings_count":0}],"findings":[{"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-052920-094949 resolves to 'Theory and Diagnostics of Hot Star Mass Loss'. A reader following the printed text alone cannot reach it.","detected_doi":"10.1146/annurev-astro-052920-094949","detected_arxiv_id":null,"ref_index":88,"audited_at":"2026-08-12T00:58:24.590379Z"},{"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 10.1051/0004-6361/202038417 resolves to 'A dynamical and radiation semi-analytical model of pulsar-star colliding winds along the orbit: Application to LS 5039'. A reader following the printed text alone cannot reach it.","detected_doi":"10.1051/0004-6361/202038417","detected_arxiv_id":null,"ref_index":92,"audited_at":"2026-08-12T00:58:24.590379Z"},{"detector":"doi_compliance","finding_type":"unresolvable_identifier","severity":"critical","verdict_class":"cross_source","note":"Identifier '10.1142/9789813226609' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","detected_doi":"10.1142/9789813226609","detected_arxiv_id":null,"ref_index":21,"audited_at":"2026-08-12T00:58:24.590379Z"},{"detector":"doi_compliance","finding_type":"unresolvable_identifier","severity":"critical","verdict_class":"cross_source","note":"Identifier '10.3847/2041-8213/ae2b' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","detected_doi":"10.3847/2041-8213/ae2b","detected_arxiv_id":null,"ref_index":69,"audited_at":"2026-08-12T00:58:24.590379Z"},{"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 (10.3847/2041-8213/aaad64) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.3847/2041-8213/aaad64","detected_arxiv_id":null,"ref_index":104,"audited_at":"2026-08-12T00:58:24.590379Z"}],"snapshot_sha256":"ad0806cacaba7228d8562353fdd0fab3c98f8857213924da1c7c3c844c87056d"},"events":[{"event_id":19244,"event_type":"pith.integrity.v1","payload_sha256":"39cddb6336965c9e420a4e609152551464d16d4390ab6d28517c76c169127f09","signature_b64":"bmNxAMZtJGN4ULtsHf3XbAW8t1NWIVdAe+uCkUdsFxhYkx3L1ciRoXE++uxldqfPL3iAyDi/WYwQyu6TzBagBw==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-12T00:58:33.871381+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.3847/2041-8213/aaad64) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. Cantiello et al., ”A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations”, Astroph. J. Letters 854 (2018): L31. https://doi.org/10.3847/2041- 8213/aaad64","arxiv_id":"2608.07951","detector":"doi_compliance","evidence":{"ref_index":104,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"10.3847/2041-","reconstructed_doi":"10.3847/2041-8213/aaad64"},"severity":"advisory","ref_index":104,"audited_at":"2026-08-12T00:58:24.590379Z","event_type":"pith.integrity.v1","detected_doi":"10.3847/2041-8213/aaad64","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"6041bbebe16b3cb63bec13633466f0dc788621661849a5628ee980ad8746b2cc","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null}},{"event_id":19243,"event_type":"pith.integrity.v1","payload_sha256":"273ae9b7e2f1d8a71f1dd3b54003a8d668056cb8396af23380a91dd83d65fd4f","signature_b64":"f+iog+pje30/6l6kwa5j78J+fAMtH7zYuqPunJOyAoajtvrZ+SasHccDMekGcbxl0pbJkJe2u6e1xPjBxs7BCA==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-12T00:58:33.863007+00:00","payload":{"note":"DOI is split by whitespace or line breaks in the printed bibliography. Reconstructed DOI 10.1051/0004-6361/202038417 resolves to 'A dynamical and radiation semi-analytical model of pulsar-star colliding winds along the orbit: Application to LS 5039'. A reader following the printed text alone cannot reach it.","snippet":"E. Molina and V. Bosch-Ramon, ”A dynamical and radi- ation semi-analytical model of pulsar-star colliding wind s along the orbit: Application to LS 5039”, Astron. As- trophys. 641 (2020): A84. https://doi.org/10.1051/0004- 6361/202038417","arxiv_id":"2608.07951","detector":"doi_compliance","evidence":{"ref_index":92,"verdict_class":"incontrovertible","resolved_title":"A dynamical and radiation semi-analytical model of pulsar-star colliding winds along the orbit: Application to LS 5039","printed_excerpt":"10.1051/0004-","reconstructed_doi":"10.1051/0004-6361/202038417"},"severity":"advisory","ref_index":92,"audited_at":"2026-08-12T00:58:24.590379Z","event_type":"pith.integrity.v1","detected_doi":"10.1051/0004-6361/202038417","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"a087db40fcde8c080e7fe98daa5bfee80b87bf45c20a461b002cfc29467dd8cb","paper_version":1,"verdict_class":"incontrovertible","resolved_title":"A dynamical and radiation semi-analytical model of pulsar-star colliding winds along the orbit: Application to LS 5039","detector_version":"1.1.0","detected_arxiv_id":null}},{"event_id":19242,"event_type":"pith.integrity.v1","payload_sha256":"041622067f5b96f589c01537b16d984cd4f94a66cc41aff495cc4b5ce745ce3f","signature_b64":"6PdmULC9ZjzN5xe3UC4/NtAahGMhxbmIsuRThKl2KhkLipRG2Zh6M3wQE0lrpbMzTRHgdA8I9Ff0EWGbx7O6Bg==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-12T00:58:33.853988+00:00","payload":{"note":"DOI is split by whitespace or line breaks in the printed bibliography. Reconstructed DOI 10.1146/annurev-astro-052920-094949 resolves to 'Theory and Diagnostics of Hot Star Mass Loss'. A reader following the printed text alone cannot reach it.","snippet":"J. S. Vink, ”Theory and Diagnostics of Hot Star Mass Loss”, Annual Review of Astronomy and Astrophysics 60 (2022): 203. https://doi.org/10.1146/annurev-astro- 052920-094949","arxiv_id":"2608.07951","detector":"doi_compliance","evidence":{"ref_index":88,"verdict_class":"incontrovertible","resolved_title":"Theory and Diagnostics of Hot Star Mass Loss","printed_excerpt":"10.1146/annurev-astro-","reconstructed_doi":"10.1146/annurev-astro-052920-094949"},"severity":"advisory","ref_index":88,"audited_at":"2026-08-12T00:58:24.590379Z","event_type":"pith.integrity.v1","detected_doi":"10.1146/annurev-astro-052920-094949","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"b97f2b7fc941072c46a66a87ea1a45034bba17dff0010926e410ac9bd36d00c3","paper_version":1,"verdict_class":"incontrovertible","resolved_title":"Theory and Diagnostics of Hot Star Mass Loss","detector_version":"1.1.0","detected_arxiv_id":null}},{"event_id":19241,"event_type":"pith.integrity.v1","payload_sha256":"e1770ec5fb47f27a9e9027ae17867e40a97d5de5140cd0e5dd0f72c0036a781c","signature_b64":"PbfNqTTkPmQfpXiLCqVFb42W+ypXSaIkjKhnnM59LcTBXy1/7tkCOzoEYN5d3Gr9jp+HvcUuLttVNcYI/ZgqBw==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-12T00:58:33.787623+00:00","payload":{"note":"Identifier '10.3847/2041-8213/ae2b' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"I. Bartos and Z. Haiman, ”Accretion is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway”, The As- trophysical Journal Letters 996, no. 2 (2026): L44. https://doi.org/10.3847/2041-8213/ae2bﬀ","arxiv_id":"2608.07951","detector":"doi_compliance","evidence":{"doi":"10.3847/2041-8213/ae2b","arxiv_id":null,"ref_index":69,"raw_excerpt":"I. Bartos and Z. Haiman, ”Accretion is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway”, The As- trophysical Journal Letters 996, no. 2 (2026): L44. https://doi.org/10.3847/2041-8213/ae2bﬀ","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":69,"audited_at":"2026-08-12T00:58:24.590379Z","event_type":"pith.integrity.v1","detected_doi":"10.3847/2041-8213/ae2b","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"f4216c8b40467e4c7c215d99da10a2126f66a3c7c097e1306664499653fe431a","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null}},{"event_id":19240,"event_type":"pith.integrity.v1","payload_sha256":"a49063fa5414c9a3b42da3fd0e83bb154d14deaec579249a81e1f0466b030b18","signature_b64":"KKdRt3vioHakywnuesHJPI5YW8/UVzDcFaltnT82qp6hUa22LVMs1b14blHxQkdE46VemxgD45+ZYGNd550OAA==","signing_key_id":"pith-v1-2026-05","created_at":"2026-08-12T00:58:33.778871+00:00","payload":{"note":"Identifier '10.1142/9789813226609' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"M. Kramer, ”Pulsars as probes of grav- ity and fundamental physics”, The Four- teenth Marcel Grossmann Meeting, (2017): 82. https://doi.org/10.1142/9789813226609 0006","arxiv_id":"2608.07951","detector":"doi_compliance","evidence":{"doi":"10.1142/9789813226609","arxiv_id":null,"ref_index":21,"raw_excerpt":"M. Kramer, ”Pulsars as probes of grav- ity and fundamental physics”, The Four- teenth Marcel Grossmann Meeting, (2017): 82. https://doi.org/10.1142/9789813226609 0006","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":21,"audited_at":"2026-08-12T00:58:24.590379Z","event_type":"pith.integrity.v1","detected_doi":"10.1142/9789813226609","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"ccab8b039d30201df2263a40b12ada32e513dd50571c0480b73a3baa5d513c3f","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null}}],"endpoint_self":"/pith/2608.07951/integrity.json","protocol_url":"https://pith.science/pith-integrity-protocol"}