English

In-Orbit Performance of the Hard X-ray Detector on board Suzaku

Astrophysics 2015-06-24 v1

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.

Keywords

Cite

@article{arxiv.astro-ph/0611233,
  title  = {In-Orbit Performance of the Hard X-ray Detector on board Suzaku},
  author = {M. Kokubun and K. Makishima and T. Takahashi and T. Murakami and M. Tashiro and Y. Fukazawa and T. Kamae and G. M. Madejski and K. Nakazawa and K. Yamaoka and Y. Terada and D. Yonetoku and S. Watanabe and T. Tamagawa and T. Mizuno and A. Kubota and N. Isobe and I. Takahashi and G. Sato and H. Takahashi and S. Hong and M. Kawaharada and N. Kawano and T. Mitani and M. Murashima and M. Suzuki and K. Abe and R. Miyawaki and M. Ohno and T. Tanaka and T. Yanagida and T. Itoh and K. Ohnuki and K. Tamura and Y. Endo and S. Hirakuri and T. Hiruta and T. Kitaguchi and T. Kishishita and S. Sugita and T. Takahashi and S. Takeda and T. Enoto and A. Hirasawa and J. Katsuta and S. Matsumura and K. Onda and M. Sato and M. Ushio and S. Ishikawa and K. Murase and H. Odaka and M. Suzuki and Y. Yaji and S. Yamada and T. Yamasaki and T. Yuasa},
  journal= {arXiv preprint arXiv:astro-ph/0611233},
  year   = {2015}
}

Comments

45 pages, 40 figures and 9 tables; accepted for Pulications of the Astronomical Society of Japan