{"schema":"pith.reference-change-event.v1","doi":"10.1103/physrevlett.131.041002","canonical_url":"https://pith.science/event/10.1103/physrevlett.131.041002","json_url":"https://pith.science/event/10.1103/physrevlett.131.041002.json","not_a_judgment":"This page records that a citing paper's bibliography includes a work with a published notice. It is not a judgment on the citing paper.","primary":{"event_id":160646,"doi":"10.1103/physrevlett.131.041002","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-07-28","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","work_arxiv_id":null,"notice_doi":"10.1103/physrevlett.131.041002","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1103/physrevlett.131.041002","json_href":"/event/10.1103/physrevlett.131.041002.json"},"events":[{"event_id":160646,"doi":"10.1103/physrevlett.131.041002","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-07-28","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","work_arxiv_id":null,"notice_doi":"10.1103/physrevlett.131.041002","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1103/physrevlett.131.041002","json_href":"/event/10.1103/physrevlett.131.041002.json"}],"flags":[{"id":734,"status":"open","status_label":"Open","citing_arxiv_id":"2207.03764","citing_title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","ref_index":95,"evidence_raw":"G. J. Feldman and R. D. Cousins, Physical review D 57, 3873 (1998). 1 Supplemental Materials Detailed Event Rates TABLE S1. Number of events remaining after each stage of event selection criteria described in the main text. Selection description Events after selection All triggers 1 .1 × 108 Analysis time hold-offs 6 .0 × 107 Single scatter 1 .0 × 107 Region-of-interest 1 .8 × 105 Analysis cuts for accidentals 3 .1 × 104 Fiducial volume 416 OD and Skin vetoes 335 T uned Detector and Xenon Response Model Details The LZ detector and xenon response models are implemented in a nest-based application that includes effects such as curved electron drift paths from field non-uniformities, finite position reconstruction resolution in the transverse (x, y) and longitudinal z directions, and position-dependence in S1 and S2 areas. The key numerical parameters of the nest model are provided in Table S2. Additionally, a header file for nest 2.3.7 that will reproduce the ER and NR response models used in this analysis is available online at https://doi.org/10.1103/PhysRevLett.131.041002. Note that the extraction field number is known to be an effective value due to multiple models for this effec","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/734","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2207.03764","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":737,"status":"open","status_label":"Open","citing_arxiv_id":"2410.00755","citing_title":"Model-independent searches of new physics in DARWIN with a semi-supervised deep learning pipeline","ref_index":74,"evidence_raw":"L.Z. collaboratiom, Physical Review Letters 131(4) (2023). DOI 10.1103/physrevlett.131.041002. URL http: //dx.doi.org/10.1103/PhysRevLett.131.041002","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/737","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2410.00755","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":736,"status":"open","status_label":"Open","citing_arxiv_id":"2503.11769","citing_title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","ref_index":1,"evidence_raw":"Aalbers, J., Akerib, D. S., Akerlof, C. W., et al. 2023, PhRvL, 131, 041002, doi: 10.1103/PhysRevLett.131.041002","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/736","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2503.11769","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":735,"status":"open","status_label":"Open","citing_arxiv_id":"2511.16394","citing_title":"Search for Higgsinos in final states with low-momentum lepton-track pairs at 13 TeV","ref_index":22,"evidence_raw":"LZ Collaboration, “First dark matter search results from the LUX-ZEPLIN (LZ) experiment”,Phys. Rev. Lett.131(2023) 041002, doi:10.1103/PhysRevLett.131.041002","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/735","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2511.16394","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":733,"status":"open","status_label":"Open","citing_arxiv_id":"2512.10513","citing_title":"A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems","ref_index":27,"evidence_raw":"J. Aalberset al.[LZ], Phys. Rev. Lett.131, no.4, 041002 (2023) doi:10.1103/PhysRevLett.131.041002 [arXiv:2207.03764 [hep-ex]]","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/733","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2512.10513","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":732,"status":"open","status_label":"Open","citing_arxiv_id":"2604.12787","citing_title":"Dark matter heating of Planet 9, and its observational implications","ref_index":37,"evidence_raw":": Dark Matter Search Result s from the CDMS II Experiment. Science 327(5973), 1619 (2010) https://doi.org/10.1126/science.1186112 arXiv:0912.3592 [astro-ph.CO] [36] Angloher, G.e.a.: Results from 730 kg days of the CRESST-II Dark Matter search. European Physical Journal C 72, 1971 (2012) https://doi.org/10.1140/epjc/s10052-012-1971-8 arXiv:1109.0 702 [astro-ph.CO] [37] Aalbers, J.e.a.: First Dark Matter Search Results from the LUX- ZEPLIN (LZ) Experiment. Phys. Rev. Lett. 131(4), 041002 (2023) https://doi.org/10.1103/PhysRevLett.131.041002 arXiv:2207.037 64 [hep-ex] [38] Stuart, E., Pardo, K.: Constraints on the dark matter-baryo n interaction cross section from galaxy cluster thermodynamics. Jo ur- nal of Cosmology and Astroparticle Physics 2026(1), 021 (2026)","evidence_cleaned":null,"evidence_source_label":"citation context","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/732","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2604.12787","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":731,"status":"open","status_label":"Open","citing_arxiv_id":"2605.04801","citing_title":"Contribution of interstellar objects to local dark matter density","ref_index":23,"evidence_raw":"Aalbers, J. and others. First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment. Phys. Rev. Lett. 2023. doi:10.1103/PhysRevLett.131.041002. arXiv:2207.03764","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-07-28","work_title":"collaboratiom, Physical Review Letters 131(4) (2023)","work_doi":"10.1103/physrevlett.131.041002","event_doi":"10.1103/physrevlett.131.041002","flag_href":"/flags/731","event_href":"/event/10.1103/physrevlett.131.041002","paper_href":"/paper/2605.04801","created_at":"2026-07-11T03:18:50.897128Z","dispute_note":null,"disputed_at":null,"disputed_by":null}],"flag_count":7,"flags_open":7,"flags_disputed":0,"desk_url":"https://pith.science/flags"}