Authors

P. S. Marrocchesi, Università degli Studi di Siena
O. Adriani, Università degli Studi di Firenze
Y. Akaike, NASA Goddard Space Flight Center
Y. Asaoka, Waseda University
E. Berti, Università degli Studi di Firenze
G. Bigongiari, Università degli Studi di Siena
M. Bongi, Università degli Studi di Firenze
P. Brogi, Università degli Studi di Siena
A. Bruno, NASA Goddard Space Flight Center
N. Cannady, NASA Goddard Space Flight Center
C. Checchia, Università degli Studi di Firenze
M. L. Cherry, Louisiana State University
G. Collazuol, Università degli Studi di Padova
A. W. Ficklin, Louisiana State University
T. G. Guzik, Louisiana State University
M. Ichimura, Hirosaki University
M. H. Israel, Washington University in St. Louis
K. Kasahara, Shibaura Institute of Technology
Y. Kawakubo, Louisiana State University
J. F. Krizmanic, NASA Goddard Space Flight Center
A. M. Messineo, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
J. W. Mitchell, NASA Goddard Space Flight Center
S. Miyake, National Institute of Technology, Ibaraki College
M. Mori, Ritsumeikan University Biwako-Kusatsu Campus
N. Mori, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
H. M. Motz, Waseda University
K. Munakata, Shinshu University
L. Pacini, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
F. Palma, Università degli Studi di Roma "Tor Vergata"
P. Papini, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
B. F. Rauch, Washington University in St. Louis
S. B. Ricciarini, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
T. Sakamoto, Aoyama Gakuin University

Document Type

Article

Publication Date

11-1-2021

Abstract

The CALorimetric Electron Telescope CALET is collecting science data on the International Space Station since October 2015 with excellent and continuous performance. Energy is measured with a deep homogeneous calorimeter (1.2 nuclear interaction lengths, 27 radiation lengths) preceded by an imaging pre-shower (3 radiation lengths, 1mm granularity) providing tracking and 10-5 electron/proton discrimination. Two independent sub-systems identify the charge Z of the incident particle from proton to iron and above (Z<40). CALET measures the cosmic-ray electron + positron flux up to 20 TeV, gamma rays up to 10 TeV, and nuclei up to the PeV scale. In this paper, we report the on-orbit performance of the instrument and summarize the main results obtained during the first 5 years of operation, including the electron + positron energy spectrum and the individual spectra of protons, heavier nuclei and iron. Solar modulation and gamma-ray observations are also concisely reported, as well as transient phenomena and the search for gravitational wave counterparts.

Publication Source (Journal or Book title)

Physics of Atomic Nuclei

First Page

985

Last Page

994

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