{"paper":{"title":"Dark Matter Search Results from a One Tonne$\\times$Year Exposure of XENON1T","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","hep-ex","hep-ph","physics.ins-det"],"primary_cat":"astro-ph.CO","authors_text":"A. Brown, A. D. Ferella, A. Di Giovanni, A. Elykov, A. Fieguth, A. Gallo Rosso, A. Kish, A. Manfredini, A. Molinario, A. P. Colijn, A. Rizzo, A. Rocchetti, B. Bauermeister, B. Kaminsky, B. Pelssers, B. Riedel, C. Capelli, C. Geis, C. Hasterok, C. Reuter, C. Tunnell, C. Weinheimer, C. Wittweg, D. Cichon, D. Coderre, D. Masson, D. Ram\\'irez Garc\\'ia, D. Schulte, D. Thers, E. Aprile, E. Brown, E. Hogenbirk, E. Shockley, F. Agostini, F. Arneodo, F. D. Amaro, F. Gao, F. Joerg, F. Lombardi, F. Piastra, F. Toschi, G. Bruno, G. Eurin, G. Koltman, G. Plante, G. Sartorelli, G. Trinchero, H. Landsman, H. Qiu, H. Simgen, H. Wang, J. Aalbers, J. A. M. Lopes, J. Conrad, J. Fei, J. Howlett, J. Mahlstedt, 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. Miller, K. Mor{\\aa}, K. Ni, L. Althueser, L. Baudis, L. Grandi, L. Levinson, L. Rauch, L. Scotto Lavina, M. Alfonsi, M. Anthony, 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, N. Priel, N. Rupp, N. Upole, O. Wack, P. A. Breur, P. de Perio, P. Di Gangi, P. Shagin, Q. Lin, R. Budnik, R. F. Lang, R. Itay, R. Podviianiuk, S. Bruenner, S. Diglio, S. Kazama, S. Lindemann, S. Reichard, S. Schindler, T. Berger, T. Marrod\\'an Undagoitia, T. Zhu, U. Oberlack, V. Pizzella, W. Fulgione, Y. Wei, Y. Zhang, Z. Greene, Z. Wang","submitted_at":"2018-05-31T17:06:59Z","abstract_excerpt":"We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \\pm 0.01)$ t, resulting in a 1.0 t$\\times$yr exposure. The energy region of interest, [1.4, 10.6] $\\mathrm{keV_{ee}}$ ([4.9, 40.9] $\\mathrm{keV_{nr}}$), exhibits an ultra-low electron recoil background rate of $(82\\substack{+5 \\\\ -3}\\textrm{ (sys)}\\pm3\\textrm{ (stat)})$ events/$(\\mathrm{t}\\times\\mathrm{yr}\\times\\mathrm{keV_{ee}})$. No significant excess over backgroun"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.12562","kind":"arxiv","version":2},"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"}