Data digitization and fluorescence signal recognition for telescope array experiment

A. Taketa; M. Fukushima; H. Ohoka; Shunsuke Ozawa; H. Sagawa; M. Takeda; H. Tokuno; S. Udo; T. Shibata; T. Matsuda; M. Tanaka; S. Ogio; Y. Tameda; J. D. Smith; S. B. Thomas

Data digitization and fluorescence signal recognition for telescope array experiment

A. Taketa, M. Fukushima, H. Ohoka, Shunsuke Ozawa, H. Sagawa, M. Takeda, H. Tokuno, S. Udo, T. Shibata, T. Matsuda, M. Tanaka, S. Ogio, Y. Tameda, J. D. Smith, S. B. Thomas

研究成果: Conference contribution

11 被引用数 (Scopus)

抄録

We have developed and made a test run of the Telescope Array (TA) Fluorescence Detector (FD) electronics. In this paper, we introduce TAFD signal processing and the method of separation of fluorescence and night sky back ground light, especially signal digitizing and one photomultiplier tube (PMT) level signal recognition board, we call as Signal Digitizer and Finder (SDF).

本文言語	English
ホスト出版物のタイトル	29th International Cosmic Ray Conference, ICRC 2005
出版社	Tata Institute of Fundamental Research
ページ	209-212
ページ数	4
巻	8
出版ステータス	Published - 2005
外部発表	はい
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India 継続期間: 2005 8月 3 → 2005 8月 10

Other

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

ASJC Scopus subject areas

核物理学および高エネルギー物理学

他のファイルとリンク

引用スタイル

Taketa, A., Fukushima, M., Ohoka, H., Ozawa, S., Sagawa, H., Takeda, M., Tokuno, H., Udo, S., Shibata, T., Matsuda, T., Tanaka, M., Ogio, S., Tameda, Y., Smith, J. D., & Thomas, S. B. (2005). Data digitization and fluorescence signal recognition for telescope array experiment. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 8, pp. 209-212). Tata Institute of Fundamental Research.

Taketa, A, Fukushima, M, Ohoka, H, Ozawa, S, Sagawa, H, Takeda, M, Tokuno, H, Udo, S, Shibata, T, Matsuda, T, Tanaka, M, Ogio, S, Tameda, Y, Smith, JD & Thomas, SB 2005, Data digitization and fluorescence signal recognition for telescope array experiment. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 8, Tata Institute of Fundamental Research, pp. 209-212, 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 05/8/3.

@inproceedings{d087a3180712404390c63119d64257d8,

title = "Data digitization and fluorescence signal recognition for telescope array experiment",

abstract = "We have developed and made a test run of the Telescope Array (TA) Fluorescence Detector (FD) electronics. In this paper, we introduce TAFD signal processing and the method of separation of fluorescence and night sky back ground light, especially signal digitizing and one photomultiplier tube (PMT) level signal recognition board, we call as Signal Digitizer and Finder (SDF).",

author = "A. Taketa and M. Fukushima and H. Ohoka and Shunsuke Ozawa and H. Sagawa and M. Takeda and H. Tokuno and S. Udo and T. Shibata and T. Matsuda and M. Tanaka and S. Ogio and Y. Tameda and Smith, {J. D.} and Thomas, {S. B.}",

year = "2005",

language = "English",

volume = "8",

pages = "209--212",

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 - Data digitization and fluorescence signal recognition for telescope array experiment

AU - Taketa, A.

AU - Fukushima, M.

AU - Ohoka, H.

AU - Ozawa, Shunsuke

AU - Sagawa, H.

AU - Takeda, M.

AU - Tokuno, H.

AU - Udo, S.

AU - Shibata, T.

AU - Matsuda, T.

AU - Tanaka, M.

AU - Ogio, S.

AU - Tameda, Y.

AU - Smith, J. D.

AU - Thomas, S. B.

PY - 2005

Y1 - 2005

N2 - We have developed and made a test run of the Telescope Array (TA) Fluorescence Detector (FD) electronics. In this paper, we introduce TAFD signal processing and the method of separation of fluorescence and night sky back ground light, especially signal digitizing and one photomultiplier tube (PMT) level signal recognition board, we call as Signal Digitizer and Finder (SDF).

AB - We have developed and made a test run of the Telescope Array (TA) Fluorescence Detector (FD) electronics. In this paper, we introduce TAFD signal processing and the method of separation of fluorescence and night sky back ground light, especially signal digitizing and one photomultiplier tube (PMT) level signal recognition board, we call as Signal Digitizer and Finder (SDF).

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UR - http://www.scopus.com/inward/citedby.url?scp=71749116850&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:71749116850

VL - 8

SP - 209

EP - 212

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 -

Data digitization and fluorescence signal recognition for telescope array experiment

抄録

Other

ASJC Scopus subject areas

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