• Title of article

    Calorimetric electron telescope (CALET) for the Japanese Exposure Facility on the ISS Original Research Article

  • Author/Authors

    K. Yoshida، نويسنده , , S. Torii، نويسنده , , N. Tateyama، نويسنده , , T. Tamura، نويسنده , , T. Ouchi، نويسنده , , T. Kashiwagi، نويسنده , , K. Hibino، نويسنده , , J. Nishimura، نويسنده , , T. Yamagami، نويسنده , , Y. Saito، نويسنده , , H. Murakami، نويسنده , , T. Kobayashi، نويسنده , , Y. Komori، نويسنده , , K. Kasahara، نويسنده , , T. Yuda، نويسنده , , M. Ohnishi، نويسنده , , M. Shibata، نويسنده , , F. Makino، نويسنده ,

  • Issue Information
    دوهفته نامه با شماره پیاپی سال 2001
  • Pages
    6
  • From page
    681
  • To page
    686
  • Abstract
    The CALET (CALorimetric Electron Telescope) instrument is proposed for the observation of TeV electrons at the Japanese Experiment Module Exposure Facility (JEM/EF) on the ISS, which is composed of an imaging calorimeter with scintillating fibers and lead plates, and a total absorption calorimeter with BGO logs. Since TeV electrons could reach only from the nearby sources within a distance less than 1 kpc, we can expect that the energy spectrum has a structural component and the arrival directions show an anisotropy. Therefore, we should be able to localize and identify the nearby cosmic-ray sources by the TeV electron observation. We report the status of development of the CALET instrument, which has a capability to observe electrons up to 10 TeV and a proton rejection power of ∼ 106. We expect to observe ∼ 103 events over 1 TeV during the 3 years observation. By using the excellent imaging capability of the CALET, gamma-rays over the GeV region and the nuclear components up to 1015 eV might also be observed.
  • Journal title
    Advances in Space Research
  • Serial Year
    2001
  • Journal title
    Advances in Space Research
  • Record number

    1127355