Antonis Leisos A sea top infrastructure for calibrating an underwater neutrino telescope the calibration principle using atmospheric showers the calibration.
Status of the EEE telescopes in Catania Paola La Rocca II Conferenza dei Progetti del Centro Fermi Rome - April 20th, 2012.
G-2 accelerator and cryo needs Mary Convery Muon Campus Review 1/23/13.
Underground Laboratories and Low Background Experiments Pia Loaiza Laboratoire Souterrain de Modane Bordeaux, March 16 th, 2006.
Status of Ultra-low Energy HPGe Detector for low-mass WIMP search Li Xin (Tsinghua University) KIMS collaboration Oct.22nd, 2005.
B. Lee Roberts, P5: 27 March 2006 - p. 1/25 Muon (g-2) to 0.25 ppm B. Lee Roberts on behalf of the New Muon (g-2) Collaboration: E969.
2003-04-25 79th KPS meeting 1 WIMP Search with CsI(Tl) Crystals – Status and Future The Future of Dark Matter Detection Y.D. Kim ( KIMS collaboration )
Optical Sensor and DAQ in IceCube Albrecht Karle University of Wisconsin-Madison [email protected] Chiba July, 2003.
Yang Yang Underground Lab in Korea (Y2L) Li Jin IHEP/ Tsinghua Beijing, China OCPA 2008, HongKong.
Studies of the Scintillation and Ionization Properties of Liquid Xenon for Dark Matter Detection Aaron Manalaysay Dept. of Physics, University of Florida.
1 Seasonal variations of the muon flux seen by the muon detector BUST 1 Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of.
Status of KIMS S.S. Myung (SNU) For the KIMS Collaboration Results from 4 crystal array Status of 12 crystal array.
