1 Retrospect of GALLEX / GNO Till Kirsten Max-Planck-Institut für Kernphysik Heidelberg / Germany 1Retrospect 2Recent update 3Why did we stop?
Conference Impressions John Bahcall (jnb) NeSS02, 9/21/02.
XMASS
Retrospect of GALLEX / GNO
XMASS ・ Physics motivation of XMASS ・ R&D using １００ｋｇ detector ・ Next step: 800 kg detector Kamioka observatory, ICRR, Univ. of Tokyo M. Nakahata for XMASS.
