pith. sign in

arxiv: 1708.07051 · v1 · pith:CPKR3FPUnew · submitted 2017-08-23 · 🌌 astro-ph.IM · astro-ph.CO· hep-ex· physics.ins-det

The XENON1T Dark Matter Experiment

XENON Collaboration: E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , M. Anthony , B. Antunes , F. Arneodo
show 136 more authors
M. Balata P. Barrow L. Baudis B. Bauermeister M. L. Benabderrahmane T. Berger A. Breskin P. A. Breur A. Brown E. Brown S. Bruenner G. Bruno R. Budnik L. B\"utikofer J. Calv\'en J. M. R. Cardoso M. Cervantes A. Chiarini D. Cichon D. Coderre A. P. Colijn J. Conrad R. Corrieri J. P. Cussonneau M. P. Decowski P. de Perio P. Di Gangi A. Di Giovanni S. Diglio J.-M. Disdier M. Doets E. Duchovni G. Eurin J. Fei A. D. Ferella A. Fieguth D. Florin D. Front W. Fulgione A. Gallo Rosso M. Galloway F. Gao M. Garbini C. Geis K.-L. Giboni L. W. Goetzke L. Grandi Z. Greene C. Grignon C. Hasterok E. Hogenbirk C. Huhmann R. Itay A. James B. Kaminsky S. Kazama G. Kessler A. Kish H. Landsman R. F. Lang D. Lellouch L. Levinson Q. Lin S. Lindemann M. Lindner F. Lombardi J. A. M. Lopes R. Maier A. Manfredini I. Maris T. Marrod\'an Undagoitia J. Masbou F. V. Massoli D. Masson D. Mayani M. Messina K. Micheneau A. Molinario K. Mor{\aa} M. Murra J. Naganoma K. Ni U. Oberlack D. Orlandi R. Othegraven P. Pakarha S. Parlati B. Pelssers R. Persiani F. Piastra J. Pienaar V. Pizzella M.-C. Piro G. Plante N. Priel D. Ram\'irez Garc\'ia L. Rauch S. Reichard C. Reuter A. Rizzo S. Rosendahl N. Rupp J. M. F. dos Santos R. Saldahna G. Sartorelli M. Scheibelhut S. Schindler J. Schreiner M. Schumann L. Scotto Lavina M. Selvi P. Shagin E. Shockley M. Silva H. Simgen M. v. Sivers M. Stern A. Stein D. Tatananni L. Tatananni D. Thers A. Tiseni G. Trinchero C. Tunnell N. Upole M. Vargas O. Wack R. Walet H. Wang Z. Wang Y. Wei C. Weinheimer C. Wittweg J. Wulf J. Ye Y. Zhang
This is my paper
classification 🌌 astro-ph.IM astro-ph.COhep-exphysics.ins-det
keywords xenon1tdarkdetectorexperimentfirstliquidmattersubsystems
0
0 comments X
read the original abstract

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2t liquid xenon inventory, 2.0t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Photoluminescence of resin-based solder flux residue under ultraviolet excitation from 120 nm to 310 nm

    physics.ins-det 2026-05 unverdicted novelty 5.0

    All tested resin-based solder flux residues photoluminesce in the visible spectral region when exposed to VUV light.