Current status of the pre-collimator development for the ASTRO-H X-ray Telescopes

Hideyuki Mori, Yoshito Haba, Takuya Miyazawa, Akihiro Furuzawa, Yuzuru Tawara, Hideyo Kunieda, Shigeo Yamauchi, Hisamitsu Awaki, Manabu Ishida, Yoshitomo Maeda, Aya Bamba, Ryo Iizuka, Takashi Okajima, Richard Mushotzky

研究成果: Conference contribution

9 被引用数 (Scopus)


We present the current status of the pre-collimator for the stray-light reduction, mounted on the ASTRO-H X-Ray Telescopes (XRT). Since the ASTRO-H XRTs adopt the conical approximation of the Wolter-I type grazing incident optics, X-rays from a source located far from the telescope boresight create a ghost image in the detector field of view (FOV) as a stray light, and then reduce the signal-to-noise ratio even in the hard X-ray band. We thus plan to mount the pre-collimator, which is comprised of cylindrical blades aligned with each primary mirror, onto the XRTs to remove the stray light. While the pre-collimator for the Soft X-ray Telescopes is designed by the similar principle adopted for the Suzaku pre-collimator, that for the Hard X-ray Telescopes requires some trade-off studies to select an appropriate blade material. The HXT pre-collimator currently utilizes the aluminum blade with the 50 mm height and 150 μm thickness. We examined the observational effects by the hard X-ray (> 10 keV) stray light and the expected performance of the pre-collimator in some scientific cases, using a ray-tracing simulator. We found that the Galactic center may be mostly covered with the stray light from the well-known bright X-ray sources. In addition, the flux estimation of the extended X-ray emission such as the Cosmic X-ray Background is also found to have large (∼ 30%) uncertainty due to the stray light from the outside of the XRT FOV. The pre-collimator improves the situations; the stray light covering the source-free region in the Galactic center can be reduced by half and the uncertainty of the flux determination for the diffuse source decreases down to < 10%.

ホスト出版物のタイトルSpace Telescopes and Instrumentation 2010
ホスト出版物のサブタイトルUltraviolet to Gamma Ray
出版ステータスPublished - 19-10-2010
イベントSpace Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray - San Diego, CA, United States
継続期間: 28-06-201002-07-2010


名前Proceedings of SPIE - The International Society for Optical Engineering


OtherSpace Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
国/地域United States
CitySan Diego, CA

All Science Journal Classification (ASJC) codes

  • 電子材料、光学材料、および磁性材料
  • 凝縮系物理学
  • コンピュータ サイエンスの応用
  • 応用数学
  • 電子工学および電気工学


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