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 |
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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 |
巻 | 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: 23-06-2008 → 28-06-2008 |
Other
Other | Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray |
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国/地域 | France |
City | Marseille |
Period | 23-06-08 → 28-06-08 |
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