Telescope array; simulation and data analysis

N. Sakurai; S. Yoshida; Shunsuke Ozawa; A. Taketa; K. Hibino; N. Inoue; Y. Wada; K. Kasahara; R. Minagawa; T. Iguchi

Telescope array; simulation and data analysis

N. Sakurai, S. Yoshida, Shunsuke Ozawa, A. Taketa, K. Hibino, N. Inoue, Y. Wada, K. Kasahara, R. Minagawa, T. Iguchi

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Telescope Array (TA) is a EAS detector which is now building in the western desert in Utah, USA. In order to estimate the performance of TA, a detailed detector simulation is being developed in Java. The number of particles produced during the development of the EAS shower with various inclinations is calculated by COSMOS code. The detection efficiency of each detector is evaluated by using the various calibration data and the results of GEANT4 simulation. And it is taken into account in estimating the signal. The analysis methods of the EAS data are also being developed using TA simulation. This report describes the structure of our simulation code, the analysis methods and the TA performance estimation based on our simulation.

Original language	English
Title of host publication	29th International Cosmic Ray Conference, ICRC 2005
Publisher	Tata Institute of Fundamental Research
Pages	193-196
Number of pages	4
Volume	8
Publication status	Published - 2005
Externally published	Yes
Event	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: 2005 Aug 3 → 2005 Aug 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
Country/Territory	India
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

Nuclear and High Energy Physics

Cite this

@inproceedings{9ec5d7fb7604413488f48dff5410594d,

title = "Telescope array; simulation and data analysis",

abstract = "Telescope Array (TA) is a EAS detector which is now building in the western desert in Utah, USA. In order to estimate the performance of TA, a detailed detector simulation is being developed in Java. The number of particles produced during the development of the EAS shower with various inclinations is calculated by COSMOS code. The detection efficiency of each detector is evaluated by using the various calibration data and the results of GEANT4 simulation. And it is taken into account in estimating the signal. The analysis methods of the EAS data are also being developed using TA simulation. This report describes the structure of our simulation code, the analysis methods and the TA performance estimation based on our simulation.",

author = "N. Sakurai and S. Yoshida and Shunsuke Ozawa and A. Taketa and K. Hibino and N. Inoue and Y. Wada and K. Kasahara and R. Minagawa and T. Iguchi",

year = "2005",

language = "English",

volume = "8",

pages = "193--196",

booktitle = "29th International Cosmic Ray Conference, ICRC 2005",

publisher = "Tata Institute of Fundamental Research",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

TY - GEN

T1 - Telescope array; simulation and data analysis

AU - Sakurai, N.

AU - Yoshida, S.

AU - Ozawa, Shunsuke

AU - Taketa, A.

AU - Hibino, K.

AU - Inoue, N.

AU - Wada, Y.

AU - Kasahara, K.

AU - Minagawa, R.

AU - Iguchi, T.

PY - 2005

Y1 - 2005

N2 - Telescope Array (TA) is a EAS detector which is now building in the western desert in Utah, USA. In order to estimate the performance of TA, a detailed detector simulation is being developed in Java. The number of particles produced during the development of the EAS shower with various inclinations is calculated by COSMOS code. The detection efficiency of each detector is evaluated by using the various calibration data and the results of GEANT4 simulation. And it is taken into account in estimating the signal. The analysis methods of the EAS data are also being developed using TA simulation. This report describes the structure of our simulation code, the analysis methods and the TA performance estimation based on our simulation.

AB - Telescope Array (TA) is a EAS detector which is now building in the western desert in Utah, USA. In order to estimate the performance of TA, a detailed detector simulation is being developed in Java. The number of particles produced during the development of the EAS shower with various inclinations is calculated by COSMOS code. The detection efficiency of each detector is evaluated by using the various calibration data and the results of GEANT4 simulation. And it is taken into account in estimating the signal. The analysis methods of the EAS data are also being developed using TA simulation. This report describes the structure of our simulation code, the analysis methods and the TA performance estimation based on our simulation.

UR - http://www.scopus.com/inward/record.url?scp=84899012004&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84899012004&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84899012004

VL - 8

SP - 193

EP - 196

BT - 29th International Cosmic Ray Conference, ICRC 2005

PB - Tata Institute of Fundamental Research

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Telescope array; simulation and data analysis

Abstract

Other

ASJC Scopus subject areas

Other files and links

Fingerprint

Cite this