Construction, test and calibration of the GLAST silicon tracker

C. Sgrò; W. B. Atwood; L. Baldini; G. Barbiellini; R. Bellazzini; F. Belli; E. Bonamente; T. Borden; J. Bregeon; A. Brez; M. Brigida; G. A. Caliandro; C. Cecchi; J. Cohen-Tanugi; A. De Angelis; P. Drell; C. Favuzzi; Y. Fukazawa; P. Fusco; F. Gargano; S. Germani; N. Giglietto; F. Giordano; T. Himel; M. Hirayama; R. P. Johnson; H. Katagiri; J. Kataoka; N. Kawai; W. Kroeger; M. Kuss; L. Latronico; F. Longo; F. Loparco; P. Lubrano; M. M. Massai; M. N. Mazziotta; M. Minuti; T. Mizuno; A. Morselli; D. Nelson; M. Nordby; T. Ohsugi; N. Omodei; M. Ozaki; M. Pepe; S. Rainò; R. Rando; M. Razzano; D. Rich; H. F.W. Sadrozinski; G. Scolieri; G. Spandre; P. Spinelli; M. Sugizaki; H. Tajima; H. Takahashi; T. Takahashi; S. Yoshida; C. Young; M. Ziegler

doi:10.1016/j.nima.2007.08.224

Construction, test and calibration of the GLAST silicon tracker

C. Sgrò^*, W. B. Atwood, L. Baldini, G. Barbiellini, R. Bellazzini, F. Belli, E. Bonamente, T. Borden, J. Bregeon, A. Brez, M. Brigida, G. A. Caliandro, C. Cecchi, J. Cohen-Tanugi, A. De Angelis, P. Drell, C. Favuzzi, Y. Fukazawa, P. Fusco, F. GarganoS. Germani, N. Giglietto, F. Giordano, T. Himel, M. Hirayama, R. P. Johnson, H. Katagiri, J. Kataoka, N. Kawai, W. Kroeger, M. Kuss, L. Latronico, F. Longo, F. Loparco, P. Lubrano, M. M. Massai, M. N. Mazziotta, M. Minuti, T. Mizuno, A. Morselli, D. Nelson, M. Nordby, T. Ohsugi, N. Omodei, M. Ozaki, M. Pepe, S. Rainò, R. Rando, M. Razzano, D. Rich, H. F.W. Sadrozinski, G. Scolieri, G. Spandre, P. Spinelli, M. Sugizaki, H. Tajima, H. Takahashi, T. Takahashi, S. Yoshida, C. Young, M. Ziegler

^*この論文の責任著者

教養教育学系

研究成果: ジャーナルへの寄稿 › 学術論文 › 査読

3 被引用数 (Scopus)

抄録

The Gamma-ray Large Area Space Telescope represents a great advance in space application of silicon detectors. With a surface of 80 m² and about 1 M readout channels it is the largest silicon tracker ever built for a space experiment. GLAST is an astro-particle mission that will study the mostly unexplored, high energy (20 MeV-300 GeV) spectrum coming from active sources or diffused in the Universe. The detector integration and test phase is complete. The full instrument underwent environmental testing and the spacecraft integration phase has just started: the launch is foreseen in late 2007. In the meanwhile the spare modules are being used for instrument calibration and performance verification employing the CERN accelerator complex. A Calibration Unit has been exposed to photon, electron and hadron beams from a few GeV up to 300 GeV. We report on the status of the instrument and on the calibration campaign.

本文言語	英語
ページ（範囲）	9-13
ページ数	5
ジャーナル	Nuclear Inst. and Methods in Physics Research, A
巻	583
号	1
DOI	https://doi.org/10.1016/j.nima.2007.08.224
出版ステータス	出版済み - 2007/12/11

ASJC Scopus 主題領域

核物理学および高エネルギー物理学
器械工学

文献へのアクセス

10.1016/j.nima.2007.08.224

引用スタイル

Sgrò, C., Atwood, W. B., Baldini, L., Barbiellini, G., Bellazzini, R., Belli, F., Bonamente, E., Borden, T., Bregeon, J., Brez, A., Brigida, M., Caliandro, G. A., Cecchi, C., Cohen-Tanugi, J., De Angelis, A., Drell, P., Favuzzi, C., Fukazawa, Y., Fusco, P., ... Ziegler, M. (2007). Construction, test and calibration of the GLAST silicon tracker. Nuclear Inst. and Methods in Physics Research, A, 583(1), 9-13. https://doi.org/10.1016/j.nima.2007.08.224

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title = "Construction, test and calibration of the GLAST silicon tracker",

abstract = "The Gamma-ray Large Area Space Telescope represents a great advance in space application of silicon detectors. With a surface of 80 m2 and about 1 M readout channels it is the largest silicon tracker ever built for a space experiment. GLAST is an astro-particle mission that will study the mostly unexplored, high energy (20 MeV-300 GeV) spectrum coming from active sources or diffused in the Universe. The detector integration and test phase is complete. The full instrument underwent environmental testing and the spacecraft integration phase has just started: the launch is foreseen in late 2007. In the meanwhile the spare modules are being used for instrument calibration and performance verification employing the CERN accelerator complex. A Calibration Unit has been exposed to photon, electron and hadron beams from a few GeV up to 300 GeV. We report on the status of the instrument and on the calibration campaign.",

keywords = "Beam test, Calibration, Gamma-ray, Silicon, Tracker",

author = "C. Sgr{\`o} and Atwood, {W. B.} and L. Baldini and G. Barbiellini and R. Bellazzini and F. Belli and E. Bonamente and T. Borden and J. Bregeon and A. Brez and M. Brigida and Caliandro, {G. A.} and C. Cecchi and J. Cohen-Tanugi and {De Angelis}, A. and P. Drell and C. Favuzzi and Y. Fukazawa and P. Fusco and F. Gargano and S. Germani and N. Giglietto and F. Giordano and T. Himel and M. Hirayama and Johnson, {R. P.} and H. Katagiri and J. Kataoka and N. Kawai and W. Kroeger and M. Kuss and L. Latronico and F. Longo and F. Loparco and P. Lubrano and Massai, {M. M.} and Mazziotta, {M. N.} and M. Minuti and T. Mizuno and A. Morselli and D. Nelson and M. Nordby and T. Ohsugi and N. Omodei and M. Ozaki and M. Pepe and S. Rain{\`o} and R. Rando and M. Razzano and D. Rich and Sadrozinski, {H. F.W.} and G. Scolieri and G. Spandre and P. Spinelli and M. Sugizaki and H. Tajima and H. Takahashi and T. Takahashi and S. Yoshida and C. Young and M. Ziegler",

year = "2007",

month = dec,

day = "11",

doi = "10.1016/j.nima.2007.08.224",

language = "英語",

volume = "583",

pages = "9--13",

journal = "Nuclear Inst. and Methods in Physics Research, A",

issn = "0168-9002",

publisher = "Elsevier B.V.",

number = "1",

}

Sgrò, C, Atwood, WB, Baldini, L, Barbiellini, G, Bellazzini, R, Belli, F, Bonamente, E, Borden, T, Bregeon, J, Brez, A, Brigida, M, Caliandro, GA, Cecchi, C, Cohen-Tanugi, J, De Angelis, A, Drell, P, Favuzzi, C, Fukazawa, Y, Fusco, P, Gargano, F, Germani, S, Giglietto, N, Giordano, F, Himel, T, Hirayama, M, Johnson, RP, Katagiri, H, Kataoka, J, Kawai, N, Kroeger, W, Kuss, M, Latronico, L, Longo, F, Loparco, F, Lubrano, P, Massai, MM, Mazziotta, MN, Minuti, M, Mizuno, T, Morselli, A, Nelson, D, Nordby, M, Ohsugi, T, Omodei, N, Ozaki, M, Pepe, M, Rainò, S, Rando, R, Razzano, M, Rich, D, Sadrozinski, HFW, Scolieri, G, Spandre, G, Spinelli, P, Sugizaki, M, Tajima, H, Takahashi, H, Takahashi, T, Yoshida, S, Young, C & Ziegler, M 2007, 'Construction, test and calibration of the GLAST silicon tracker', Nuclear Inst. and Methods in Physics Research, A, vol. 583, no. 1, pp. 9-13. https://doi.org/10.1016/j.nima.2007.08.224

TY - JOUR

T1 - Construction, test and calibration of the GLAST silicon tracker

AU - Sgrò, C.

AU - Atwood, W. B.

AU - Baldini, L.

AU - Barbiellini, G.

AU - Bellazzini, R.

AU - Belli, F.

AU - Bonamente, E.

AU - Borden, T.

AU - Bregeon, J.

AU - Brez, A.

AU - Brigida, M.

AU - Caliandro, G. A.

AU - Cecchi, C.

AU - Cohen-Tanugi, J.

AU - De Angelis, A.

AU - Drell, P.

AU - Favuzzi, C.

AU - Fukazawa, Y.

AU - Fusco, P.

AU - Gargano, F.

AU - Germani, S.

AU - Giglietto, N.

AU - Giordano, F.

AU - Himel, T.

AU - Hirayama, M.

AU - Johnson, R. P.

AU - Katagiri, H.

AU - Kataoka, J.

AU - Kawai, N.

AU - Kroeger, W.

AU - Kuss, M.

AU - Latronico, L.

AU - Longo, F.

AU - Loparco, F.

AU - Lubrano, P.

AU - Massai, M. M.

AU - Mazziotta, M. N.

AU - Minuti, M.

AU - Mizuno, T.

AU - Morselli, A.

AU - Nelson, D.

AU - Nordby, M.

AU - Ohsugi, T.

AU - Omodei, N.

AU - Ozaki, M.

AU - Pepe, M.

AU - Rainò, S.

AU - Rando, R.

AU - Razzano, M.

AU - Rich, D.

AU - Sadrozinski, H. F.W.

AU - Scolieri, G.

AU - Spandre, G.

AU - Spinelli, P.

AU - Sugizaki, M.

AU - Tajima, H.

AU - Takahashi, H.

AU - Takahashi, T.

AU - Yoshida, S.

AU - Young, C.

AU - Ziegler, M.

PY - 2007/12/11

Y1 - 2007/12/11

N2 - The Gamma-ray Large Area Space Telescope represents a great advance in space application of silicon detectors. With a surface of 80 m2 and about 1 M readout channels it is the largest silicon tracker ever built for a space experiment. GLAST is an astro-particle mission that will study the mostly unexplored, high energy (20 MeV-300 GeV) spectrum coming from active sources or diffused in the Universe. The detector integration and test phase is complete. The full instrument underwent environmental testing and the spacecraft integration phase has just started: the launch is foreseen in late 2007. In the meanwhile the spare modules are being used for instrument calibration and performance verification employing the CERN accelerator complex. A Calibration Unit has been exposed to photon, electron and hadron beams from a few GeV up to 300 GeV. We report on the status of the instrument and on the calibration campaign.

AB - The Gamma-ray Large Area Space Telescope represents a great advance in space application of silicon detectors. With a surface of 80 m2 and about 1 M readout channels it is the largest silicon tracker ever built for a space experiment. GLAST is an astro-particle mission that will study the mostly unexplored, high energy (20 MeV-300 GeV) spectrum coming from active sources or diffused in the Universe. The detector integration and test phase is complete. The full instrument underwent environmental testing and the spacecraft integration phase has just started: the launch is foreseen in late 2007. In the meanwhile the spare modules are being used for instrument calibration and performance verification employing the CERN accelerator complex. A Calibration Unit has been exposed to photon, electron and hadron beams from a few GeV up to 300 GeV. We report on the status of the instrument and on the calibration campaign.

KW - Beam test

KW - Calibration

KW - Gamma-ray

KW - Silicon

KW - Tracker

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U2 - 10.1016/j.nima.2007.08.224

DO - 10.1016/j.nima.2007.08.224

M3 - 学術論文

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EP - 13

JO - Nuclear Inst. and Methods in Physics Research, A

JF - Nuclear Inst. and Methods in Physics Research, A

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ER -

Construction, test and calibration of the GLAST silicon tracker

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