CALET Results after Three Years on Orbit on the International Space Station

P. Maestro; O. Adriani; Y. Akaike; Y. Asaoka; E. Berti; G. Bigongiari; M. Bongi; P. Brogi; A. Bruno; N. Cannady; C. Checchia; M. L. Cherry; G. Collazuol; T. G. Guzik; M. Ichimura; M. H. Israel; K. Kasahara; Y. Kawakubo; J. F. Krizmanic; P. S. Marrocchesi; A. M. Messineo; J. W. Mitchell; S. Miyake; M. Mori; N. Mori; H. M. Motz; K. Munakata; L. Pacini; F. Palma; P. Papini; B. F. Rauch; S. B. Ricciarini; T. Sakamoto; M. Sasaki; F. Stolzi; A. Sulaj; T. Tamura; S. Torii; J. P. Wefel; K. Yoshida

doi:10.1134/S1063778819660384

CALET Results after Three Years on Orbit on the International Space Station

作者: Maestro P.¹^,2, Adriani O.³^,4, Akaike Y.⁵^,3, Asaoka Y.⁶^,7, Berti E.³^,4, Bigongiari G.¹^,2, Bongi M.³^,4, Brogi P.¹^,2, Bruno A.⁸, Cannady N.⁵^,3, Checchia C.³^,4, Cherry M.L.⁹, Collazuol G.⁹^,10, Guzik T.G.⁹, Ichimura M.¹¹, Israel M.H.³, Kasahara K.¹², Kawakubo Y.⁹, Krizmanic J.F.⁵^,3, Marrocchesi P.S.¹^,2, Messineo A.M.²^,13, Mitchell J.W.¹⁴, Miyake S.¹⁵, Mori M.¹⁶, Mori N.⁴, Motz H.M.¹⁷, Munakata K.¹⁸, Pacini L.⁴, Palma F.¹⁹^,20, Papini P.⁴, Rauch B.F.³, Ricciarini S.B.⁴^,21, Sakamoto T.²², Sasaki M.⁵^,3, Stolzi F.¹^,2, Sulaj A.¹^,2, Tamura T.²³, Torii S.⁶^,7^,24, Wefel J.P.⁹, Yoshida K.¹², ¹²
隶属关系:
1. Department of Physical Sciences, Earth and Environment
2. INFN Sezione di Pisa
3. Department of Physics
4. INFN Sezione di Florence
5. CRESST and Astroparticle Physics Laboratory NASA/GSFC
6. Research Institute for Science and Engineering
7. Human Spaceflight Technology Directorate, Japan Aerospace Exploration Agency
8. Heliospheric Science Division
9. Department of Physics and Astronomy
10. INFN Sezione di Padova
11. Faculty of Science and Technology, Graduate School of Science and Technology
12. Department of Electronic Information Systems
13. University of Pisa
14. Astroparticle Physics Laboratory, NASA/GSFC
15. Department of Electrical and Electronic Systems Engineering
16. Department of Physical Sciences, College of Science and Engineering
17. International Center for Science and Engineering Programs
18. Faculty of Science
19. University of Rome “Tor Vergata”
20. INFN Sezione di Rome “Tor Vergata”
21. Institute of Applied Physics (IFAC)
22. College of Science and Engineering, Department of Physics and Mathematics
23. Kanagawa University
24. School of Advanced Science and Engineering
期: 卷 82, 编号 6 (2019)
页面: 766-772
栏目: Elementary Particles and Fields
URL: https://journals.rcsi.science/1063-7788/article/view/194884
DOI: https://doi.org/10.1134/S1063778819660384
ID: 194884

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The 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 γ 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 identification 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.

Email: paolo.maestro@pi.infn.it

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CALET Results after Three Years on Orbit on the International Space Station

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