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Abstract
Xenon dual-phase time projection chambers designed to search for weakly interacting massive particles have so far shown a relative energy resolution which degrades with energy above 200 keV due to the saturation effects. This has limited their sensitivity in the search for rare events like the neutrinoless double-beta decay of at its Q value, . For the XENON1T dual-phase time projection chamber, we demonstrate that the relative energy resolution at is as low as () % in its one-ton fiducial mass, and for single-site interactions at . We also present a new signal correction method to rectify the saturation effects of the signal readout system, resulting in more accurate position reconstruction and indirectly improving the energy resolution. The very good result achieved in XENON1T opens up new windows for the xenon dual-phase dark matter detectors to simultaneously search for other rare events.
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1 Columbia University, Physics Department, New York, USA (GRID:grid.21729.3f) (ISNI:0000000419368729)
2 Stockholm University, AlbaNova, Department of Physics, Oskar Klein Centre, Stockholm, Sweden (GRID:grid.10548.38) (ISNI:0000 0004 1936 9377)
3 University of Bologna and INFN-Bologna, Department of Physics and Astronomy, Bologna, Italy (GRID:grid.6292.f) (ISNI:0000 0004 1757 1758)
4 Johannes Gutenberg-Universität Mainz, Institut für Physik & Exzellenzcluster PRISMA, Mainz, Germany (GRID:grid.5802.f) (ISNI:0000 0001 1941 7111)
5 Westfälische Wilhelms-Universität Münster, Institut für Kernphysik, Münster, Germany (GRID:grid.5949.1) (ISNI:0000 0001 2172 9288)
6 University of Coimbra, LIBPhys, Department of Physics, Coimbra, Portugal (GRID:grid.8051.c) (ISNI:0000 0000 9511 4342)
7 University of Torino and INFN-Torino, INAF-Astrophysical Observatory of Torino, Department of Physics, Turin, Italy (GRID:grid.7605.4) (ISNI:0000 0001 2336 6580)
8 Nikhef and the University of Amsterdam, Amsterdam, The Netherlands (GRID:grid.7177.6) (ISNI:0000000084992262)
9 New York University Abu Dhabi, Abu Dhabi, United Arab Emirates (GRID:grid.440573.1)
10 University of Zurich, Physik-Institut, Zurich, Switzerland (GRID:grid.7400.3) (ISNI:0000 0004 1937 0650)
11 Rensselaer Polytechnic Institute, Department of Physics, Applied Physics and Astronomy, Troy, USA (GRID:grid.33647.35) (ISNI:0000 0001 2160 9198)
12 Nikhef and the University of Amsterdam, Amsterdam, The Netherlands (GRID:grid.7177.6) (ISNI:0000000084992262); Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103)
13 Weizmann Institute of Science, Department of Particle Physics and Astrophysics, Rehovot, Israel (GRID:grid.13992.30) (ISNI:0000 0004 0604 7563)
14 Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103)
15 University of Napoli and INFN-Napoli, Department of Physics “Ettore Pancini”, Naples, Italy (GRID:grid.4691.a) (ISNI:0000 0001 0790 385X)
16 Purdue University, Department of Physics and Astronomy, West Lafayette, USA (GRID:grid.169077.e) (ISNI:0000 0004 1937 2197)
17 Universität Freiburg, Physikalisches Institut, Freiburg, Germany (GRID:grid.5963.9)
18 SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes, France (GRID:grid.463940.c) (ISNI:0000 0001 0475 7658)
19 University of L’Aquila, Department of Physics and Chemistry, L’Aquila, Italy (GRID:grid.158820.6) (ISNI:0000 0004 1757 2611); INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466750.6)
20 University of Torino and INFN-Torino, INAF-Astrophysical Observatory of Torino, Department of Physics, Turin, Italy (GRID:grid.7605.4) (ISNI:0000 0001 2336 6580); INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466750.6)
21 LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3, Paris, France (GRID:grid.410511.0) (ISNI:0000 0001 2149 7878)
22 INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466750.6)
23 University of Chicago, Department of Physics and Kavli Institute for Cosmological Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822)
24 The University of Tokyo, Kamioka Observatory, Institute for Cosmic Ray Research, and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Hida, Japan (GRID:grid.26999.3d) (ISNI:0000 0001 2151 536X)
25 Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya, Japan (GRID:grid.27476.30) (ISNI:0000 0001 0943 978X)
26 Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France (GRID:grid.433124.3) (ISNI:0000 0001 0664 3574)
27 Kobe University, Department of Physics, Kobe, Japan (GRID:grid.31432.37) (ISNI:0000 0001 1092 3077)
28 Columbia University, Physics Department, New York, USA (GRID:grid.21729.3f) (ISNI:0000000419368729); Stockholm University, AlbaNova, Department of Physics, Oskar Klein Centre, Stockholm, Sweden (GRID:grid.10548.38) (ISNI:0000 0004 1936 9377)
29 University of California San Diego, Department of Physics, La Jolla, USA (GRID:grid.266100.3) (ISNI:0000 0001 2107 4242)
30 Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103); SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes, France (GRID:grid.463940.c) (ISNI:0000 0001 0475 7658)
31 Rice University, Department of Physics and Astronomy, Houston, USA (GRID:grid.21940.3e) (ISNI:0000 0004 1936 8278)
32 University of California, Physics and Astronomy Department, Los Angeles, USA (GRID:grid.19006.3e) (ISNI:0000 0000 9632 6718)