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XMASS detector

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arxiv 1301.2815 v1 pith:5WMJPHXT submitted 2013-01-13 physics.ins-det astro-ph.COastro-ph.IMhep-ex

XMASS detector

K. Abe , K. Hieda , K. Hiraide , S. Hirano , Y. Kishimoto , K. Kobayashi , S. Moriyama , K. Nakagawa
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M. Nakahata H. Nishiie H. Ogawa N. Oka H. Sekiya A. Shinozaki Y. Suzuki A. Takeda O. Takachio K. Ueshima D. Umemoto M. Yamashita B. S. Yang S. Tasaka J. Liu K. Martens K. Hosokawa K. Miuchi A. Murata Y. Onishi Y. Otsuka Y. Takeuchi Y. H. Kim K. B. Lee M. K. Lee J. S. Lee Y. Fukuda Y. Itow Y. Nishitani K. Masuda H. Takiya H. Uchida N. Y. Kim Y. D. Kim F. Kusaba D. Motoki K. Nishijima K. Fujii I. Murayama S. Nakamura
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classification physics.ins-det astro-ph.COastro-ph.IMhep-ex
keywords xmassdarkdetectormatteracquisitionaimsbetacalibration
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The XMASS project aims to detect dark matter, pp and $^{7}$Be solar neutrinos, and neutrinoless double beta decay using ultra pure liquid xenon. The first phase of the XMASS experiment searches for dark matter. In this paper, we describe the XMASS detector in detail, including its configuration, data acquisition equipment and calibration system.

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