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CALET Results After Three Years on Orbit on the International Space StationThe CALorimetric Electron Telescope (CALET) is an astroparticle physics experiment installed on the International Space Station since August 2015. The CALET mission was conceived to address several outstanding questions of high-energy astroparticle physics, like indirect detection of dark matter, the origin of cosmic rays (CRs), their mechanisms of acceleration and galactic propagation, the presence of possible nearby astrophysical CR sources. That can be achieved by precise measurements of the fluxes of CR electrons and gamma-rays up to the unexplored region above 1 TeV, and the energy spectra and composition of CR nuclei from a few tens of GeV to hundreds of TeV. In order to perform these observations, the instrument combines a thick total absorption PWO crystal calorimeter for energy measurement, a scintillator hodoscope for charge identi cation and thin imaging tungsten-scintillating fiber calorimeter providing accurate particle tracking and complementary charge measurement.

In this paper, we will present an overview of the main CALET results based on the data collected in the first three years of the mission.
Document ID
20210014031
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
P Maestro ORCID
(University of Siena Siena, Italy)
O. Adriani
(University of Florence Florence, Toscana, Italy)
E. Berti
(University of Florence Florence, Toscana, Italy)
M. Bongi
(University of Florence Florence, Toscana, Italy)
Y. Akaike
(University of Maryland, Baltimore County Baltimore, Maryland, United States)
Y. Asaoka
(Waseda University Tokyo, Japan)
G. Bigongiari
(University of Siena Siena, Italy)
P. Brogi
(University of Siena Siena, Italy)
P. S. Marrocchesi
(University of Siena Siena, Italy)
A. Bruno
(Goddard Space Flight Center Greenbelt, Maryland, United States)
N. Cannady
(Goddard Space Flight Center Greenbelt, Maryland, United States)
M. L. Cherry
(Louisiana State University Baton Rouge, Louisiana, United States)
T. G. Guzik
(Louisiana State University Baton Rouge, Louisiana, United States)
Y. Kawakubo
(Louisiana State University Baton Rouge, Louisiana, United States)
J. P. Wefel
(Louisiana State University Baton Rouge, Louisiana, United States)
M. Ichimura
(Hirosaki University Hirosaki, Japan)
M. H. Israel
(Washington University in St. Louis St Louis, Missouri, United States)
B. F. Rauch
(Washington University in St. Louis St Louis, Missouri, United States)
K. Kasahara
(Waseda University Tokyo, Japan)
J. F. Krizmanic
(Goddard Space Flight Center Greenbelt, Maryland, United States)
A. M. Messineo
(University of Pisa Pisa, Toscana, Italy)
J W Mitchell
(Goddard Space Flight Center Greenbelt, Maryland, United States)
S. Miyake
(Ibaraki National College of Technology Hitachi-Naka, Japan)
M. Mori
(Ritsumeikan University Kyoto, Japan)
N. Mori
(INFN Sezione di Firenze Sesto Fiorentino, Italy)
L. Pacini
(INFN Sezione di Firenze Sesto Fiorentino, Italy)
P. Papini
(INFN Sezione di Firenze Sesto Fiorentino, Italy)
H. M. Motz
(Shinshu University Matsumoto, Japan)
K. Munakata
(Shinshu University Matsumoto, Japan)
F. Palma
(University of Rome Tor Vergata Rome, Lazio, Italy)
S. B. Ricciarini
(Nello Carrara Institute of Applied Physics Sesto Fiorentino, Italy)
T. Sakamoto
(Aoyama Gakuin University Tokyo, Japan)
T. Tamura
(Kanagawa University Yokohama, Japan)
S. Torii
(Waseda University Tokyo, Japan)
K. Yoshida
(Shibaura Institute of Technology Tokyo, Japan)
Date Acquired
April 20, 2021
Publication Date
November 1, 2019
Publication Information
Publication: Physics of Atomic Nuclei
Publisher: Springer
Volume: 82
Issue Publication Date: February 5, 2020
ISSN: 1063-7788
e-ISSN: 1562-692X
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: 80GSFC17M0002
WBS: 399131
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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