@article{oai:repo.qst.go.jp:00045485,
 author = {Yamashita, Naoyuki and Kodaira, Satoshi and et.al and 山下 直之 and 小平 聡},
 issue = {Suppl.A},
 journal = {Journal of the Physical Society of Japan},
 month = {Apr},
 note = {The Japanese lunar explorer SELENE was launched from Tanegashima Space Center on September 14, 2007. It consists of a main orbiter KAGUYA at 100 km altitude and two daughter satellites (relay satellite OKINA and VRAD satellite OUNA) with 14 scientific instruments. The high precision gamma-ray spectrometer (GRS) on KAGUYA measures 200 keV–12 MeV gamma rays to determine the elemental composition of the lunar surface. The GRS is composed of a large Ge crystal as a main detector and massive bismuth germinate (BGO) crystals and a plastic scintillator as anticoincidence detectors. The Ge detector is cooled by a Stirling cryocooler below 90 K during the observation. After successful launch of the spacecraft and initial checkouts, the GRS started the nominal observation on December 21, 2007, and the temperatures and counting rates of the GRS were confirmed to be stable. Energy spectra of gamma rays with a good energy resolution are being obtained over the lunar surface, which will allow us to make global maps of the elemental abundances of the Moon soon.},
 pages = {153--156},
 title = {Germanium Gamma-Ray Spectrometer on SELENE (KAGUYA)},
 volume = {78},
 year = {2009}
}