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
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