{"paper":{"title":"VUV-sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A. Burenkov, A. Craycraft, A. Der Mesrobian-Kabakian, A. Dragone, A. House, A. Iverson, A. Jamil, A. Karelin, A. K. Soma, A. Kuchenkov, A. Odian, A. Piepke, A. Pocar, A. Robinson, A. Schubert, B. Cleveland, B. Mong, C. Chambers, C. Licciardi, C. T. Overman, D. Beck, D. Fairbank, D. Fudenberg, D. Harris, D. Moore, D. Qiu, D. Sinclair, D. S. Leonard, E. Brown, E. Raguzin, E. V. Hansen, E. W. Hoppe, F. Nolet, F. Reti\\`ere, F. Vachon, G. Anton, G. F. Cao, G. Gallina, G. Giacomini, G. Gratta, G. Li, G. S. Ortega, G. St-Hilaire, G. Visser, G. Wrede, I. Badhrees, I. J. Arnquist, I. Ostrovskiy, J. B. Albert, J. Dalmasson, J. Daughhetee, J. Dilling, J. Echevers, J. Farine, J.-F. Pratte, J. H\\\"o{\\ss}l, J. L. Orrell, J.-L. Vuilleumier, J. P. Brodsky, J. Schneider, J. Todd, J. Zhao, K. Murray, K. Odgers, K. Skarpaas, K. S. Kumar, L. Cao, L. Fabris, L. J. Kaufman, L. J. Wen, L. Lupin-Jimenez, L. Yang, M. Chiu, M. Coon, M. C\\^ot\\'e, M. Hasan, M. Heffner, M. Hughes, M. J. Dolinski, M. Jewell, M. Oriunno, M. Tarka, M. Wagenpfeil, M. Weber, N. Roy, O. Njoya, O. Zeldovich, P. Barbeau, P. C. Rowson, P. Hufschmidt, Q. Wang, Q. Xia, R. DeVoe, R. Fontaine, R. Gornea, R. J. Newby, R. Kr\\\"ucken, R. MacLellan, R. Saldanha, R. Tsang, S. A. Charlebois, S. Delaquis, S. Feyzbakhsh, S. J. Daugherty, S. Kravitz, S. Li, S. Parent, S. Rescia, S. Sangiorgio, S. Schmidt, S. X. Wu, T. Brunner, T. Daniels, T. Didberidze, T. Koffas, T. Michel, T. Rao, T. Rossignol, T. Stiegler, T. Tolba, T. Tsang, T. Ziegler, U. Wichoski, V. Belov, V. Radeka, V. Stekhanov, V. Veeraraghavan, W. Cree, W. Fairbank, W. H. Wu, W. R. Cen, W. Wei, X. L. Sun, X. S. Jiang, X. Zhang, Y. H. Lin, Y. Ito, Y. Lan, Y.-R. Yen, Y. Y. Ding, Y. Zhou, Z. Li, Z. Ning","submitted_at":"2018-06-06T14:33:22Z","abstract_excerpt":"Future tonne-scale liquefied noble gas detectors depend on efficient light detection in the VUV range. In the past years Silicon Photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large area avalanche photodiodes. The next generation double beta decay experiment, nEXO, with a 5 tonne liquid xenon time projection chamber, will use SiPMs for detecting the $178\\,\\text{nm}$ xenon scintillation light, in order to achieve an energy resolution of $\\sigma / Q_{\\beta\\beta} = 1\\, \\%$. This paper presents recent measurements of the VUV-HD generation SiPMs fr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.02220","kind":"arxiv","version":3},"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"}