{"paper":{"title":"Rapid data quality investigations of gravitational-wave events with the Data Quality Report Builder toolkit","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"The Data Quality Report Builder toolkit identifies 96% of the data problems humans found in third observing run gravitational-wave candidates.","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Adrian Helmling-Cornell, Airene Ahuja, Annudesh Liyanage, Benjamin Mannix, Beverly Berger, Caitlin Rawcliffe, Chayan Chatterjee, Christiano Palomba, Derek Davis, Dimitrios Pesios, Francesco Di Renzo, Franz Herbst, Hirotaka Yuzurihara, Jess McIver, Joseph Areeda, Julian Ding, Man Leong Chan, Marissa Walker, Max Trevor, Nicolas Arnaud, Olivia Godwin, Paolina Doliva, Philippe Nguyen, Rachael Huxford, Raymond Frey, Raymond Ng, Robert Schofield, Ronaldas Macas, Sofia Alvarez-Lopez, Sophie Perry, Viola Sordini, Yannick Lecoeuche, Zach Yarbrough","submitted_at":"2026-05-15T17:03:40Z","abstract_excerpt":"We present the Data Quality Report Builder toolkit, DQRbuild, a suite of data quality tools that have been developed to vet gravitational-wave events in preparation for the fourth LIGO-Virgo-KAGRA observing run. We explain the main functionality and the many scientific tests that we support. To validate the performance of the tools included in the toolkit, we run a series of tests on all significant candidates shared as public alerts in the third observing run to compare against what was manually reported using human intervention. We find that these automated tools can now identify 96% of the "},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"We find that these automated tools can now identify 96% of the problems identified by humans during this previous observing run, with a 24% false alarm rate.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The set of scientific tests implemented in DQRbuild will continue to capture the majority of data quality issues that arise in the fourth observing run in the same way they did for O3 candidates.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"DQRbuild toolkit automates data quality vetting for gravitational-wave events, recovering 96% of human-identified issues from O3 with a 24% false alarm rate.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"The Data Quality Report Builder toolkit identifies 96% of the data problems humans found in third observing run gravitational-wave candidates.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"ca8d16a6987e25b2f21162211edc472dfa264e322c3ed2294a3b5978d8aab188"},"source":{"id":"2605.16183","kind":"arxiv","version":1},"verdict":{"id":"f2a9ebf7-cba1-4af9-aa12-36d339498fc5","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-19T18:23:23.660069Z","strongest_claim":"We find that these automated tools can now identify 96% of the problems identified by humans during this previous observing run, with a 24% false alarm rate.","one_line_summary":"DQRbuild toolkit automates data quality vetting for gravitational-wave events, recovering 96% of human-identified issues from O3 with a 24% false alarm rate.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The set of scientific tests implemented in DQRbuild will continue to capture the majority of data quality issues that arise in the fourth observing run in the same way they did for O3 candidates.","pith_extraction_headline":"The Data Quality Report Builder toolkit identifies 96% of the data problems humans found in third observing run gravitational-wave candidates."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.16183/integrity.json","findings":[],"available":true,"detectors_run":[{"name":"doi_title_agreement","ran_at":"2026-05-19T18:31:18.733059Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"doi_compliance","ran_at":"2026-05-19T18:31:09.043107Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"cited_work_retraction","ran_at":"2026-05-19T17:52:01.526804Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"citation_quote_validity","ran_at":"2026-05-19T17:49:47.142736Z","status":"skipped","version":"0.1.0","findings_count":0},{"name":"ai_meta_artifact","ran_at":"2026-05-19T17:33:30.681947Z","status":"skipped","version":"1.0.0","findings_count":0},{"name":"external_links","ran_at":"2026-05-19T17:31:43.345786Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"claim_evidence","ran_at":"2026-05-19T16:41:55.418408Z","status":"completed","version":"1.0.0","findings_count":0}],"snapshot_sha256":"2f42fcf399ec73b49ebcc2db88ada71d025897c5646f731a84df4c4c8f6b9013"},"references":{"count":96,"sample":[{"doi":"","year":null,"title":"Capoteet al., Advanced LIGO detector performance in the fourth observing run, Phys","work_id":"3de2c276-b6a8-4b77-8c3e-d5f5404a9adc","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":null,"title":"Acernese Fet al.(VIRGO) 2023J. Phys. Conf. Ser.2429012040","work_id":"c6d5cbc5-a89f-414c-964f-6bae939cd4b5","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":null,"title":"Abe Het al.(KAGRA) 2023PTEP202310A101 (Preprint2203.07011)","work_id":"2f8de0f3-5428-433c-958d-4bb1b16bafe1","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":null,"title":"Observation of Gravitational Waves from a Binary Black Hole Merger","work_id":"ab878228-151c-4a29-8026-a4308b076d30","ref_index":4,"cited_arxiv_id":"1602.03837","is_internal_anchor":true},{"doi":"","year":null,"title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","work_id":"a19136e8-99c2-49be-b029-60af2e20c6ee","ref_index":5,"cited_arxiv_id":"1710.05832","is_internal_anchor":true}],"resolved_work":96,"snapshot_sha256":"3183bee7639bcba71b7587e16f04ae74fdbb722cd1b9a9200b94842158d52e59","internal_anchors":24},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}