Soft X-ray calibration for the NeXT X-ray Telescope

Yoshitomo Maeda, Takayuki Hayashi, Hideyuki Mori, Ryoko Nakamura, Takuro Satoh, Akiko Sekiguchi, Kentaro Someya, Kensuke Tamura, Manabu Ishida, Takeyuki Osawa, Takayuki Shirata, Masaki Suzuki, Yasushi Ogasaka, Akihiro Furuzawa, Yoshito Haba, Takuya Miyazawa, Hideyo Kunieda, Koujun Yamashita, Takashi Okajima

研究成果: Conference contribution

3 被引用数 (Scopus)

抄録

We present a plan on soft X-ray calibration for the New Exploration X-ray Telescope (NeXT). Two hard and two soft X-ray telescopes (HXTs/SXTs: see Ogasaka et al. 2008 in this volume) provide images up to 80 keV with a large effective area. Following to the Suzaku X-ray telescope, the mirrors on SXTs are tightly nested to maximize the aperture efficiency. To illuminate the mirrors at all, we plan to adopt a raster scan system using a pencil beam collimated from an X-ray generator. We summarize a current status of the soft X-ray ground calibration system at ISAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.

本文言語English
ホスト出版物のタイトルSpace Telescopes and Instrumentation 2008
ホスト出版物のサブタイトルUltraviolet to Gamma Ray
7011
DOI
出版ステータスPublished - 01-12-2008
外部発表はい
イベントSpace Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille, France
継続期間: 23-06-200828-06-2008

Other

OtherSpace Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
国/地域France
CityMarseille
Period23-06-0828-06-08

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

フィンガープリント

「Soft X-ray calibration for the NeXT X-ray Telescope」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル