Expected performance of CALET

K. Kasahara, S. Torii, Y. Shimizu, Y. Akaike, K. Taira, K. Yoshida, I. Watanabe

Research output: Contribution to conferencePaper

1 Citation (Scopus)

Abstract

CALET is a detector planned to be on board ISS to investigate high energy universe by observing high energy gamma-rays, electrons and other cosmic ray. It is now in the phase A/B study period of the JAXA program. The performance of CALET was studied earlier[1] but the design structure (mainly its size) has been changed since that time. We have been performing new M.C simulations corresponding to the new structure to evaluate its basic performance. This is to report some of the new results.

Original languageEnglish
Pages1433-1436
Number of pages4
Publication statusPublished - 2007 Jan 1
Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
Duration: 2007 Jul 32007 Jul 11

Conference

Conference30th International Cosmic Ray Conference, ICRC 2007
CountryMexico
CityMerida, Yucatan
Period07/7/307/7/11

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ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Kasahara, K., Torii, S., Shimizu, Y., Akaike, Y., Taira, K., Yoshida, K., & Watanabe, I. (2007). Expected performance of CALET. 1433-1436. Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.