15 July 2008 Soft x-ray calibration for the NeXT x-ray telescope
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Abstract
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.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yoshitomo Maeda, Yoshitomo Maeda, Takayuki Hayashi, Takayuki Hayashi, Hideyuki Mori, Hideyuki Mori, Ryoko Nakamura, Ryoko Nakamura, Takuro Satoh, Takuro Satoh, Akiko Sekiguchi, Akiko Sekiguchi, Kentaro Someya, Kentaro Someya, Kensuke Tamura, Kensuke Tamura, Manabu Ishida, Manabu Ishida, Takeyuki Osawa, Takeyuki Osawa, Takayuki Shirata, Takayuki Shirata, Masaki Suzuki, Masaki Suzuki, Yasushi Ogasaka, Yasushi Ogasaka, Akihiro Furuzawa, Akihiro Furuzawa, Yoshito Haba, Yoshito Haba, Takuya Miyazawa, Takuya Miyazawa, Hideyo Kunieda, Hideyo Kunieda, Koujun Yamashita, Koujun Yamashita, Takashi Okajima, Takashi Okajima, } "Soft x-ray calibration for the NeXT x-ray telescope", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 70112O (15 July 2008); doi: 10.1117/12.788652; https://doi.org/10.1117/12.788652
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