High-energy astroparticle physics with CALET
Paolo Maestro

TL;DR
CALET is a space-based instrument designed to measure high-energy cosmic rays, aiming to search for dark matter, understand cosmic-ray acceleration, and identify astrophysical sources, with expected high-resolution energy measurements from GeV to TeV energies.
Contribution
This paper reviews the design, configuration, and expected performance of CALET, highlighting its capabilities in cosmic-ray measurement and astrophysical research.
Findings
Instrument design allows charge identification from Z=1 to 40.
Energy measurement resolution is excellent from a few GeV to several hundred TeV.
Expected to provide valuable data for dark matter and cosmic-ray studies.
Abstract
The CALorimetric Electron Telescope (CALET) will be installed on the Exposure Facility of the Japanese Experiment Module (JEM-EF) on the International Space Station (ISS) in 2014 where it will measure the cosmic-ray fluxes for five years. Its main scientific goals are to search for dark matter, investigate the mechanism of cosmic-ray acceleration and propagation in the Galaxy and discover possible astrophysical sources of high-energy electrons nearby the Earth. The instrument, under construction, consists of two layers of segmented plastic scintillators for the cosmic-ray charge identification (CHD), a 3 X-thick tungsten-scintillating fiber imaging calorimeter (IMC) and a 27 X-thick lead-tungstate calorimeter (TASC). The CHD can provide single-element separation in the interval of atomic number Z from 1 to 40, while IMC and TASC can measure the energy of cosmic-ray particles…
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