CALET on the International Space Station: the first three years of observations
Creators
- 1. Department of Physical Sciences, Earth and Environment, University of Siena, via Roma 56, 53100 Siena (Italy)
- 2. Department of Physics, University of Florence, Via Sansone, 1-50019 Sesto Fiorentino (Italy)
- 3. CRESST and Astroparticle Physics Laboratory NASA/GSFC, Greenbelt, MD 20771 (United States)
- 4. Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa, Chiba 277-8582 (Japan)
- 5. Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan)
- 6. Department of Physics, Washington University, One Brookings Drive, St. Louis, MO 63130-4899 (United States)
- 7. Heliospheric Science Division, NASA/Goddard Space Flight Center—Code 672, Bldg. 21, Room 137D, Greenbelt MD 20771 (United States)
- 8. Institute of Applied Physics (IFAC), National Research Council (CNR), Via Madonna del Piano, 10, 50019 Sesto Fiorentino (Italy)
- 9. Department of Physics and Astronomy, Louisiana State University, 202 Nicholson Hall, Baton Rouge, LA 70803 (United States)
- 10. Department of Physics and Astronomy, University of Padova, Via Marzolo, 8, 35131 Padova (Italy)
- 11. University of Rome 'Tor Vergata', Via della Ricerca Scientifica 1, 00133 Rome (Italy)
- 12. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa 252-5210 (Japan)
Description
The CALorimetric Electron Telescope CALET is a space instrument designed to carry out precision measurements of high energy cosmic-rays on the JEM-EF external platform on the International Space Station, where it has been collecting science data continuously since mid October 2015. In addition to its primary goal of identifying nearby sources of high-energy electrons and possible signatures of dark matter in the electron spectrum, CALET is carrying out extensive measurements of the energy spectra, relative abundances and secondary-to-primary ratios of elements from proton to iron, and even above (up to Z = 40), studying the details of galactic particle propagation and acceleration. An overview of CALET based on the data taken during the first three years of observations is presented, including a direct measurement of the electron+positron energy spectrum from 11 GeV to 4.8 TeV. The proton spectrum has been measured from 50 GeV to 10 TeV covering, for the first time with a single space-borne instrument, the whole energy interval previously investigated in separate sub-ranges by magnetic spectrometers and calorimetric instruments. Preliminary spectra of cosmic-ray nuclei are also presented, together with gamma-ray observations and searches for an e.m. counterpart of LIGO/Virgo GW events. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1402-4896/ab957dAdditional details
Identifiers
Publishing Information
- Journal Title
- Physica Scripta (Online)
- Journal Volume
- 95
- Journal Issue
- 7
- Journal Page Range
- [9 p.]
- ISSN
- 1402-4896
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52091536
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- ACCURACY; CALORIMETRY; COSMIC RADIATION; ELECTRON SPECTRA; ENERGY SPECTRA; GAMMA RADIATION; GEV RANGE 10-100; INTERNATIONAL SPACE STATION; MAGNETIC SPECTROMETERS; NONLUMINOUS MATTER; PROTON SPECTRA; TEV RANGE 01-10
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ENERGY RANGE; GEV RANGE; IONIZING RADIATIONS; MATTER; MEASURING INSTRUMENTS; RADIATIONS; SATELLITES; SPACE VEHICLES; SPECTRA; SPECTROMETERS; TEV RANGE; VEHICLES