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      Energy Spectrum of Cosmic-ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station

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          Abstract

          First results of a cosmic-ray electron + positron spectrum, from 10 GeV to 3 TeV, is presented based upon observations with the CALET instrument on the ISS starting in October, 2015. Nearly a half million electron + positron events are included in the analysis. CALET is an all-calorimetric instrument with total vertical thickness of 30 \(X_0\) and a fine imaging capability designed to achieve a large proton rejection and excellent energy resolution well into the TeV energy region. The observed energy spectrum over 30 GeV can be fit with a single power law with a spectral index of -3.152 \(\pm\) 0.016 (stat.+ syst.). Possible structure observed above 100 GeV requires further investigation with increased statistics and refined data analysis.

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          Author and article information

          Journal
          05 December 2017
          Article
          10.1103/PhysRevLett.119.181101
          1712.01711
          7bf2c95a-38e6-4fe8-ad2a-22bad4204f9b

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          Physical Review Letters 119, 181101 (2017)
          7 pages, 6 figures, published 1 November 2017 in Physical Review Letters
          astro-ph.HE

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