Expected performance of CALET

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

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    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
    Title of host publicationProceedings of the 30th International Cosmic Ray Conference, ICRC 2007
    PublisherUniversidad Nacional Autonoma de Mexico
    Pages1433-1436
    Number of pages4
    Volume3
    EditionOG PART 2
    Publication statusPublished - 2007
    Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan
    Duration: 2007 Jul 32007 Jul 11

    Other

    Other30th International Cosmic Ray Conference, ICRC 2007
    CityMerida, Yucatan
    Period07/7/307/7/11

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

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  • Cite this

    Kasahara, K., Torii, S., Shimizu, Y., Akaike, Y., Taira, K., Yoshida, K., & Watanabe, I. (2007). Expected performance of CALET. In Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007 (OG PART 2 ed., Vol. 3, pp. 1433-1436). Universidad Nacional Autonoma de Mexico.