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

Research output: Contribution to conference › Paper › peer-review

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 language	English
Pages	1433-1436
Number of pages	4
Publication status	Published - 2007 Jan 1
Event	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: 2007 Jul 3 → 2007 Jul 11

Conference

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

ASJC Scopus subject areas

Nuclear and High Energy Physics

Cite this

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author = "K. Kasahara and S. Torii and Y. Shimizu and Y. Akaike and K. Taira and K. Yoshida and I. Watanabe",

year = "2007",

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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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M3 - Paper

AN - SCOPUS:84899495067

SP - 1433

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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

Abstract

Conference

ASJC Scopus subject areas

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