@inproceedings{oai:repo.qst.go.jp:00053582,
 author = {Yoshida, Kenji and Torii, Syoji and Kitamura, Hisashi and Uchihori, Yukio and et.al and 吉田 賢二 and 鳥居 祥二 and 北村 尚 and 内堀 幸夫},
 book = {Proceedings of International Cosmic Ray Conference},
 month = {Aug},
 note = {We are proposing the CALET (CALorimetric Electron Telescope) for the observation of high-energy electrons and gamma rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe electrons (+positrons) in 1GeV-10TeV and gamma rays in 20MeV-10TeV with a high energy resolution of 2 percent at 100GeV, an angular resolution of 0.06deg at 100GeV, and a high proton rejection power of 10^6. CALET has the geometrical factor of nearly 1m2sr and three-years observation is expected. Precise electron observation of CALET enables us to identify cosmic-ray electron sources by the detection of distinctive features in the energy spectrum and anisotropy toward nearby sources. The ISS orbit enables CALET to survey all of the sky in a wide field of view of 2 sr without attitude control of the instrument. In addition, by the hybrid observations of high-energy electrons and gamma rays, the CALET can search for WIMP dark matter.},
 title = {Observation of High-Energy Electron, Gamma Ray, and Dark Matter},
 volume = {OG},
 year = {2005}
}