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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XMASS detector

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