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

被引：2

作者：

Maeda, Yoshitonto ^{[1
]}

Hayashi, Takayuki ^{[1
]}

Mori, Hideyuki ^{[1
]}

Nakamura, Ryoko ^{[1
]}

Satoh, Takuro ^{[1
]}

Sekiguchi, Akiko ^{[1
]}

Someya, Kentaro ^{[1
]}

Tamura, Kensuke ^{[1
]}

Ishida, Manabu ^{[1
]}

Osawa, Takeyuki ^{[2
]}

Shirata, Takayuki ^{[2
]}

Suzuki, Masaki ^{[2
]}

Ogasaka, Yasushi ^{[3
]}

Furuzawa, Akhiro ^{[3
]}

Haba, Yoshito ^{[3
]}

Miyazawa, Takuya ^{[3
]}

Kunieda, Hideyo ^{[3
]}

Yamashita, Koujun ^{[3
]}

Okajima, Takashi ^{[4
]}

机构：

[1] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2298510, Japan

[2] Tokyo Metropolitan Univ, Hachioji, Tokyo 1920397, Japan

[3] Nagoya Univ, Dept Phys, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[4] NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2 | 2008年 / 7011卷

关键词：

X-ray; optics; calibration;

D O I：

10.1117/12.788652

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a plan oil soft X-ray calibration for Hie 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 oil 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, TSAS/JAXA. We also review the calibration of the Suzaku XRTs since the optics are very similar to the NeXT SXTs.

引用

页数：9

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