Abstract
The in-orbit performance and calibration of the Hard X-ray Detector (HXD) on board the X-ray astronomy satellite Suzaku are described. Its basic performances, including a wide energy bandpass of 10-600 keV, energy resolutions of ∼ 4 keV (FWHM) at 40 keV and ∼ 11% at 511 keV, and a high background rejection efficiency, have been confirmed by extensive in-orbit calibrations. The long-term gains of PIN-Si diodes have been stable within 1% for half a year, and those of scintillators have decreased by 5-20%. The residual non-X-ray background of the HXD is the lowest among past non-imaging hard X-ray instruments in energy ranges of 15-70 and 150-500 keV. We provide accurate calibrations of energy responses, angular responses, timing accuracy of the HXD, and relative normalizations to the X-ray CCD cameras using multiple observations of the Crab Nebula.
| Original language | English |
|---|---|
| Journal | Publications of the Astronomical Society of Japan |
| Volume | 59 |
| Issue number | 1 SPEC. ISS. |
| Publication status | Published - 2007 |
| Externally published | Yes |
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Keywords
- Instrumentation: detectors
- X-rays: general
- X-rays: individual (Crab Nebula)
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Cite this
In-orbit performance of the hard X-ray detector on board Suzaku. / Kokubun, Motohide; Makishima, Kazuo; Takahashi, Tadayuki; Murakami, Toshio; Tashiro, Makoto; Fukazawa, Yasushi; Kamae, Tuneyoshi; Madejski, Greg M.; Nakazawa, Kazuhiro; Yamaoka, Kazutaka; Terada, Yukikatsu; Yonetoku, Daisuke; Watanabe, Shin; Tamagawa, Toru; Mizuno, Tsunefumi; Kubota, Aya; Isobe, Naoki; Takahashi, Isao; Sato, Goro; Takahashi, Hiromitsu; Hong, Soojing; Kawaharada, Madoka; Kawano, Naomi; Mitani, Takefumi; Murashima, Mio; Suzuki, Masaya; Abe, Keiichi; Miyawaki, Ryouhei; Ohno, Masanori; Tanaka, Takaaki; Yanagida, Takayuki; Itoh, Takeshi; Ohnuki, Kousuke; Tamura, Ken Ichi; Endo, Yasuhiko; Hirakuri, Shinya; Hiruta, Tatsuro; Kitaguchi, Takao; Kishishita, Tetsuichi; Sugita, Satoshi; Takahashi, Takuya; Takeda, Shin'ichiro; Enoto, Teruaki; Hirasawa, Ayumi; Katsuta, Jun'ichiro; Matsumura, Satoshi; Onda, Kaori; Sato, Mitsuhiro; Ushio, Masayoshi; Ishikawa, Shin Nosuke; Murase, Koichi; Odaka, Hirokazu; Suzuki, Masanobu; Yaji, Yuichi; Yamada, Shinya; Yamasaki, Tomonori; Yuasa, Takayuki.
In: Publications of the Astronomical Society of Japan, Vol. 59, No. 1 SPEC. ISS., 2007.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - In-orbit performance of the hard X-ray detector on board Suzaku
AU - Kokubun, Motohide
AU - Makishima, Kazuo
AU - Takahashi, Tadayuki
AU - Murakami, Toshio
AU - Tashiro, Makoto
AU - Fukazawa, Yasushi
AU - Kamae, Tuneyoshi
AU - Madejski, Greg M.
AU - Nakazawa, Kazuhiro
AU - Yamaoka, Kazutaka
AU - Terada, Yukikatsu
AU - Yonetoku, Daisuke
AU - Watanabe, Shin
AU - Tamagawa, Toru
AU - Mizuno, Tsunefumi
AU - Kubota, Aya
AU - Isobe, Naoki
AU - Takahashi, Isao
AU - Sato, Goro
AU - Takahashi, Hiromitsu
AU - Hong, Soojing
AU - Kawaharada, Madoka
AU - Kawano, Naomi
AU - Mitani, Takefumi
AU - Murashima, Mio
AU - Suzuki, Masaya
AU - Abe, Keiichi
AU - Miyawaki, Ryouhei
AU - Ohno, Masanori
AU - Tanaka, Takaaki
AU - Yanagida, Takayuki
AU - Itoh, Takeshi
AU - Ohnuki, Kousuke
AU - Tamura, Ken Ichi
AU - Endo, Yasuhiko
AU - Hirakuri, Shinya
AU - Hiruta, Tatsuro
AU - Kitaguchi, Takao
AU - Kishishita, Tetsuichi
AU - Sugita, Satoshi
AU - Takahashi, Takuya
AU - Takeda, Shin'ichiro
AU - Enoto, Teruaki
AU - Hirasawa, Ayumi
AU - Katsuta, Jun'ichiro
AU - Matsumura, Satoshi
AU - Onda, Kaori
AU - Sato, Mitsuhiro
AU - Ushio, Masayoshi
AU - Ishikawa, Shin Nosuke
AU - Murase, Koichi
AU - Odaka, Hirokazu
AU - Suzuki, Masanobu
AU - Yaji, Yuichi
AU - Yamada, Shinya
AU - Yamasaki, Tomonori
AU - Yuasa, Takayuki
PY - 2007
Y1 - 2007
N2 - The in-orbit performance and calibration of the Hard X-ray Detector (HXD) on board the X-ray astronomy satellite Suzaku are described. Its basic performances, including a wide energy bandpass of 10-600 keV, energy resolutions of ∼ 4 keV (FWHM) at 40 keV and ∼ 11% at 511 keV, and a high background rejection efficiency, have been confirmed by extensive in-orbit calibrations. The long-term gains of PIN-Si diodes have been stable within 1% for half a year, and those of scintillators have decreased by 5-20%. The residual non-X-ray background of the HXD is the lowest among past non-imaging hard X-ray instruments in energy ranges of 15-70 and 150-500 keV. We provide accurate calibrations of energy responses, angular responses, timing accuracy of the HXD, and relative normalizations to the X-ray CCD cameras using multiple observations of the Crab Nebula.
AB - The in-orbit performance and calibration of the Hard X-ray Detector (HXD) on board the X-ray astronomy satellite Suzaku are described. Its basic performances, including a wide energy bandpass of 10-600 keV, energy resolutions of ∼ 4 keV (FWHM) at 40 keV and ∼ 11% at 511 keV, and a high background rejection efficiency, have been confirmed by extensive in-orbit calibrations. The long-term gains of PIN-Si diodes have been stable within 1% for half a year, and those of scintillators have decreased by 5-20%. The residual non-X-ray background of the HXD is the lowest among past non-imaging hard X-ray instruments in energy ranges of 15-70 and 150-500 keV. We provide accurate calibrations of energy responses, angular responses, timing accuracy of the HXD, and relative normalizations to the X-ray CCD cameras using multiple observations of the Crab Nebula.
KW - Instrumentation: detectors
KW - X-rays: general
KW - X-rays: individual (Crab Nebula)
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UR - http://www.scopus.com/inward/citedby.url?scp=34047176366&partnerID=8YFLogxK
M3 - Article
VL - 59
JO - Publication of the Astronomical Society of Japan
JF - Publication of the Astronomical Society of Japan
SN - 0004-6264
IS - 1 SPEC. ISS.
ER -