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論文・著書情報
タイトル |
和文: | |
英文: | Design and Performance of the Wide-Field X-Ray Monitor on Board the High-Energy Transient Explorer 2 |
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著者 |
和文: |
Shirasaki, Y.,
河合 誠之,
Yoshida, A.,
Matsuoka, M.,
Tamagawa, T.,
Torii, K.,
Sakamoto, T.,
Suzuki, M.,
Urata, Y.,
Sato, R.,
Nakagawa, Y.,
Takahashi, D.,
Fenimore, E. E.,
Galassi, M.,
Lamb, D. Q.,
Graziani, C.,
Donaghy, T. Q.,
Vanderspek, R.,
Yamauchi, M.,
Takagishi, K.,
Hatsukade, I..
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英文: |
Shirasaki, Y.,
Kawai, N.,
Yoshida, A.,
Matsuoka, M.,
Tamagawa, T.,
Torii, K.,
Sakamoto, T.,
Suzuki, M.,
Urata, Y.,
Sato, R.,
Nakagawa, Y.,
Takahashi, D.,
Fenimore, E. E.,
Galassi, M.,
Lamb, D. Q.,
Graziani, C.,
Donaghy, T. Q.,
Vanderspek, R.,
Yamauchi, M.,
Takagishi, K.,
Hatsukade, I..
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言語 |
English |
掲載誌/書名 |
和文: | |
英文: | Publications of the Astronomical Society of Japan |
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巻, 号, ページ
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Vol. 55
pp. 1033-1049
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出版年月 |
2003年10月 |
出版者 |
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会議名称 |
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開催地 |
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DOI |
https://doi.org/10.1093/pasj/55.5.1033 |
アブストラクト |
The Wide-field X-ray Monitor (WXM) is one of the scientific instruments carried on the High Energy Transient Explorer 2 (HETE-2) satellite launched on 2000 October 9. HETE-2 is an international mission consisting of a small satellite dedicated to provide broad-band observations and accurate localizations of gamma-ray bursts (GRBs). A unique feature of this mission is its capability to determine and transmit GRB coordinates in almost real-time through the burst alert network. The WXM consists of three elements: four identical Xe-filled one-dimensional position-sensitive proportional counters, two sets of one-dimensional coded apertures, and the main electronics. The WXM counters are sensitive to X-rays between 2keV and 25keV within a field-of-view of about 1.5sr, with a total detector area of about 350 cm2. The in-flight triggering and localization capability can produce a real-time GRB location of several to 30arcmin accuracy, with a limiting sensitivity of 10<s up>-7 erg cm-2. In this report, the details of the mechanical structure, electronics, on-board software, ground and in-flight calibration, and in-flight performance of the WXM are discussed. |
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