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STELLAR CHEMISTRY
CALET makes direct measurements of cosmic-ray electron spectrum
by Staff Writers
Tokyo, Japan (SPX) Jul 23, 2018

The Calorimetric Electron Telescope (CALET) instrument mounted externally to the ISS on the Japanese Experimental Module Kibo

An international team of researchers succeeded in extending their result from a previous study and directly measured the cosmic-ray all-electron (electron + positron) spectrum in an energy range from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope (CALET).

CALET, a detector optimized to observe high-energy electrons, was installed on the Japanese Experimental Module Kibo on the International Space Station (ISS) on August 2015 as the first, Japanese-led, space-based mission dedicated to cosmic ray observations. Intended for a long-term operation, CALET has been accumulating data since October 2015.

"I have been told that the international scientific community is interested in the observations by CALET because one of our objectives is to understand the origin of high-energy cosmic rays and the nature of dark matter, some of the most profound mysteries in this universe," says Professor Shoji Torii of Waseda University, the principal investigator of the CALET mission.

The origin and acceleration of cosmic rays are not yet well known, and cosmic-ray electrons are one of the priority targets of high-energy cosmic ray research. Precise measurements of electrons above 1 TeV have been difficult to achieve because they require high-precision energy measurements of the cosmic-ray particles, sensitivity to detect the rare electron flux, and capability of accurate electron identification from the more than 1,000 times higher flux of protons in the TeV energy region.

"The long-term observations on the ISS and the calorimeter of CALET's capabilities, such as being able to identify the charge of incident particles, detect incident direction, and measure the particle energy and identify the species by detecting the particle shower development, have enabled our team to perform accurate measurements of cosmic-ray electrons into the TeV region," Professor Torii explains.

Previously in November 2017, the team reported their first result in measuring the cosmic-ray electrons in the energy range from 10 GeV to 3 TeV in Physical Review Letters.

In this recent study, they developed a new data analysis method to maximize detection at higher energies, approximately doubling the statistics compared to their previous study and allowing CALET to obtain high-precision measurements of cosmic-ray electron spectrum up to 4.8 TeV.

Professor Torii says that the statistics will improve nearly three times more than now by using data after a five-year observation. "It will also reduce systematic uncertainties, including that from the detector response.

"Our ultimate goal is to push the energy limit up to 20 TeV and obtain the precise energy spectrum, in which there is a high probability of discovering nearby astrophysical cosmic-ray resources or revealing the nature of dark matter."

This study was published in online in Physical Review Letters on June 25, 2018.

Research Report: Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station


Related Links
Waseda University
Stellar Chemistry, The Universe And All Within It


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STELLAR CHEMISTRY
Hawaii telescopes help unravel long-standing cosmic mystery
Manoa HI (SPX) Jul 16, 2018
Astronomers and physicists around the world, including in Hawaii, have begun to unravel a long-standing cosmic mystery. Using a vast array of telescopes in space and on Earth, they have identified a source of cosmic rays--highly energetic particles that continuously rain down on Earth from space. In a paper published this week in the journal Science, scientists have, for the first time, provided evidence for a known blazar, designated TXS 0506+056, as a source of high-energy neutrinos. At 8:54 p.m ... read more

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