Slide 1 XMASS ・ Physics motivation of XMASS ・ R&D using １００ｋｇ detector ・ Next step: 800 kg detector Kamioka observatory, ICRR, Univ. of Tokyo M. Nakahata…

Retrospect of GALLEX / GNO Till Kirsten Max-Planck-Institut für Kernphysik Heidelberg / Germany Retrospect Recent update 3 Why did we stop? 1 RETROSPECT GALLEX / GNO , SAGE…

Conference Impressions John Bahcall (http://www.sns.ias.edu/~jnb) NeSS02, 9/21/02 Thanks! Jordan Tom Kera NSF colleagues SOC Speakers (especially from other countries) Participants…

XMASS ・　Physics motivation of XMASS ・　R&D using １００ｋｇ detector ・　Next step: 800 kg detector Kamioka observatory, ICRR, Univ. of Tokyo M. Nakahata…

Retrospect of GALLEX / GNO Till Kirsten Max-Planck-Institut für Kernphysik Heidelberg / Germany Retrospect Recent update 3 Why did we stop? 1 RETROSPECT GALLEX / GNO , SAGE…