{"paper":{"title":"First Dark Matter Search Results from the XENON1T Experiment","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM","hep-ex","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"A. Brown, A. D. Ferella, A. Di Giovanni, A. Fieguth, A. Gallo Rosso, A. Kish, A. Manfredini, A. Molinario, A. P. Colijn, A. Rizzo, A. Stein, A. Tiseni, B. Bauermeister, B. Kaminsky, B. Pelssers, B. Riedel, C. Geis, C. Grignon, C. Hasterok, C. Reuter, C. Tunnell, C. Weinheimer, D. Cichon, D. Coderre, D. Lellouch, D. Masson, D. Mayani, D. Thers, E. Aprile, E. Brown, E. Hogenbirk, E. Shockley, F. Agostini, F. Arneodo, F. D. Amaro, F. Gao, F. Lombardi, F. Piastra, F. V. Massoli, G. Bruno, G. Eurin, G. Kessler, G. Plante, G. Sartorelli, G. Trinchero, H. Landsman, H. Simgen, H. Wang, I. Mari\\c{s}, J. Aalbers, J. A. M. Lopes, J. Calv\\'en, J. Conrad, J. Fei, J. Howlett, J. Masbou, J. M. F. dos Santos, J. M. R. Cardoso, J. Naganoma, J. P. Cussonneau, J. Pienaar, J. Schreiner, J. Wulf, J. Ye, K. Micheneau, K. Mor{\\aa}, K. Ni, L. Baudis, L. B\\\"utikofer, L. Grandi, L. Levinson, L. Rauch, L. Scotto Lavina, L. W. Goetzke, M. Alfonsi, M. Anthony, M. Cervantes, M.-C. Piro, M. Galloway, M. Garbini, M. L. Benabderrahmane, M. Lindner, M. Messina, M. Murra, M. P. Decowski, M. Scheibelhut, M. Schumann, M. Selvi, M. Silva, M. Vargas, M. v. Sivers, N. Priel, N. Rupp, N. Upole, P. A. Breur, P. Barrow, P. de Perio, P. Di Gangi, P. Pakarha, P. Shagin, Q. Lin, R. Budnik, R. F. Lang, R. Gardner, R. Itay, R. Persiani, R. Saldanha, S. Bruenner, S. Diglio, S. Kazama, S. Lindemann, S. Reichard, S. Rosendahl, S. Schindler, S. Thapa, T. Berger, T. Marrod\\'an Undagoitia, T. Zhu, U. Oberlack, V. Pizzella, W. Fulgione, Y. Wei, Y. Zhang, Z. Greene, Z. Wang","submitted_at":"2017-05-18T15:36:12Z","abstract_excerpt":"We report the first dark matter search results from XENON1T, a $\\sim$2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042$\\pm$12) kg fiducial mass and in the [5, 40] $\\mathrm{keV}_{\\mathrm{nr}}$ energy range of interest for WIMP dark matter searches, the electronic recoil background was $(1.93 \\pm 0.25) \\times 10^{-4}$ events/(kg $\\times$ day $\\times \\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.06655","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"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"}