Expected performance of CALET

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

Expected performance of CALET

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

研究成果: Paper › 査読

抄録

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.

本文言語	English
ページ	1433-1436
ページ数	4
出版ステータス	Published - 2007 1月 1
イベント	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico 継続期間: 2007 7月 3 → 2007 7月 11

Conference

Conference	30th International Cosmic Ray Conference, ICRC 2007
国/地域	Mexico
City	Merida, Yucatan
Period	07/7/3 → 07/7/11

ASJC Scopus subject areas

核物理学および高エネルギー物理学

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引用スタイル

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T1 - Expected performance of CALET

AU - Kasahara, K.

AU - Torii, S.

AU - Shimizu, Y.

AU - Akaike, Y.

AU - Taira, K.

AU - Yoshida, K.

AU - Watanabe, I.

PY - 2007/1/1

Y1 - 2007/1/1

N2 - 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.

AB - 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.

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T2 - 30th International Cosmic Ray Conference, ICRC 2007

Y2 - 3 July 2007 through 11 July 2007

ER -

Expected performance of CALET

抄録

Conference

ASJC Scopus subject areas

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