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

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

11 Citations (Scopus)

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).

Original language	English
Title of host publication	29th International Cosmic Ray Conference, ICRC 2005
Publisher	Tata Institute of Fundamental Research
Pages	209-212
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

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).

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

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

Abstract

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ASJC Scopus subject areas

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