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The CALorimetric Electron Telescope (CALET) on the International Space Station: Results from the First Two Years of Operation

Authors :
Asaoka Y
Adriani O
Akaike Y
Asano K
Bagliesi MG
Berti E
Bigongiari G
Binns WR
Bonechi S
Bongi M
Bruno A
Brogi P
Buckley J H
Cannady N
Castellini G
Checchia C
Cherry M L
Collazuol G
Di Felice V
Ebisawa K
Fuke H
Guzik T G
Hams T
Hasebe N
Hibinov K
Ichimura M
Ioka K
Ishizaki W
Israel M H
Kasahara K
Kataoka J
Kataoka R
Katayose Y
Kato C
Kawanaka N
Kawakubo Y
Kohri K
Krawczynski H S
Krizmanic J F
Lomtadze T
Maestro P
Marrocchesi P S
Messineo A M
Mitchell J W
Miyake S
Moiseev A A
Mori K
Mori M
Mori N
Motz H M
Munakata K
Murakami H
Nakahira S
Nishimura J
De Nolfo G A
Okuno S
Ormes J F
Ozawa S
Pacini L
Palma F
Pal'shin V
Papini P
Penacchioni A V
Rauch B F
Ricciarini S B
Sakai K
Sakamoto T
Sasaki M
Shimizu Y
Shiomi A
Sparvoli R
Spillantini P
Stolzi F
Sugita S
Suh J E
Sulaj A
Takahashi I
Takayanagi M
Takita M
Tamura T
Tateyama N
Terasawa T
Tomida H
Torii S
Tsunesada Y
Uchihori Y
Ueno S
Vannuccini E
Wefel J P
Yamaoka K
Yanagita S
Yoshida A
Yoshida K
Source :
EPJ Web of Conferences, Vol 208, p 13001 (2019)
Publication Year :
2019
Publisher :
EDP Sciences, 2019.

Abstract

The CALorimetric Electron Telescope (CALET) space experiment, which has been developed by Japan in collaboration with Italy and the United States, is a high-energy astroparticle physics mission on the International Space Station (ISS). The primary goals of the CALET mission include investigation of possible nearby sources of high-energy electrons, detailed study of galactic cosmic-ray acceleration and propagation, and search for dark matter signatures. With a long-term observation onboard the ISS, the CALET experiment measures the flux of cosmic-ray electrons (including positrons) up to 20 TeV, gamma-rays to 10 TeV, and nuclei up to 1,000 TeV based on its charge separation capability from Z = 1 to 40. Since the start of science operation in mid-October, 2015, a continuous observation has been maintained without any major interruptions. The number of triggered events over 10 GeV is nearly 20 million per month. By using the data obtained during the first two-years, here we present a summary of the CALET observations: 1) Electron+positron energy spectrum, 2) Nuclei analysis, 3) Gamma-ray observation with a characterization of the on-orbit performance. The search results for the electromagnetic counterparts of LIGO/Virgo gravitational wave events are also discussed.

Subjects

Subjects :
Physics
QC1-999

Details

Language :
English
ISSN :
2100014X and 11844345
Volume :
208
Database :
Directory of Open Access Journals
Journal :
EPJ Web of Conferences
Publication Type :
Academic Journal
Accession number :
edsdoj.1184434529fa416fae2be78eab3dea93
Document Type :
article
Full Text :
https://doi.org/10.1051/epjconf/201920813001