Status and performance of the CALorimetric Electron Telescope (CALET) on the international space station

[1]  B. Rauch.  Predicted CALET measurements of ultra-heavy cosmic ray relative abundances , 2014 .

[2]  A. Albert,et al.  Search for gamma-ray spectral lines with the Fermi Large Area Telescope and dark matter implications , 2013, 1305.5597.

[3]  E. Amato,et al.  Spectral breaks as a signature of cosmic ray induced turbulence in the Galaxy. , 2012, Physical review letters.

[4]  A. Basti,et al.  Beam test performance of a scintillator-based detector for the charge identification of relativistic ions , 2011 .

[5]  T Glanzman,et al.  Measurement of separate cosmic-ray electron and positron spectra with the fermi large area telescope. , 2011, Physical review letters.

[6]  V. Malvezzi,et al.  PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra , 2011, Science.

[7]  S. Torii.  Calorimetric electron telescope mission: Search for dark matter and nearby sources , 2011 .

[8]  C. J. Waddington,et al.  COSMIC RAY ORIGIN IN OB ASSOCIATIONS AND PREFERENTIAL ACCELERATION OF REFRACTORY ELEMENTS: EVIDENCE FROM ABUNDANCES OF ELEMENTS 26Fe THROUGH 34Se , 2009, 0906.2021.

[9]  G. C. Barbarino,et al.  An anomalous positron abundance in cosmic rays with energies 1.5–100 GeV , 2009, Nature.

[10]  A. Noutsos,et al.  High-energy particle acceleration in the shell of a supernova remnant , 2004, Nature.

[11]  K. Yoshida,et al.  The Most Likely Sources of High-Energy Cosmic-Ray Electrons in Supernova Remnants , 2003, astro-ph/0308470.

[12]  C. Cesarsky,et al.  The maximum energy of cosmic rays accelerated by supernova shocks , 1983 .

[13]  P. Lipari,et al.  First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5350 GeV , 2013 .