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Xtend, the Soft X-ray Imaging Telescope for the X-ray Imaging and Spectroscopy Mission (XRISM)

Authors :
Mori, Koji
Tomida, Hiroshi
Nakajima, Hiroshi
Okajima, Takashi
Noda, Hirofumi
Tanaka, Takaaki
Uchida, Hiroyuki
Hagino, Kouichi
Kobayashi, Shogo Benjamin
Suzuki, Hiromasa
Yoshida, Tessei
Murakami, Hiroshi
Uchiyama, Hideki
Nobukawa, Masayoshi
Nobukawa, Kumiko
Yoneyama, Tomokage
Matsumoto, Hironori
Tsuru, Takeshi
Yamauchi, Makoto
Hatsukade, Isamu
Ishida, Manabu
Maeda, Yoshitomo
Hayashi, Takayuki
Tamura, Keisuke
Boissay-Malaquin, Rozenn
Sato, Toshiki
Hiraga, Junko
Kohmura, Takayoshi
Yamaoka, Kazutaka
Dotani, Tadayasu
Ozaki, Masanobu
Tsunemi, Hiroshi
Kanemaru, Yoshiaki
Sato, Jin
Takaki, Toshiyuki
Terada, Yuta
Miyazaki, Keitaro
Kusunoki, Kohei
Otsuka, Yoshinori
Yokosu, Haruhiko
Yonemaru, Wakana
Asahina, Yoh
Asakura, Kazunori
Yoshimoto, Marina
Ode, Yuichi
Sato, Junya
Hakamata, Tomohiro
Aoyagi, Mio
Aoki, Yuma
Tsunomachi, Shun
Doi, Toshiki
Aoki, Daiki
Fujisawa, Kaito
Kitajima, Masatoshi
Hayashida, Kiyoshi
Source :
Proc. of SPIE vol. 12181, 121811T (2022)
Publication Year :
2023

Abstract

Xtend is a soft X-ray imaging telescope developed for the X-Ray Imaging and Spectroscopy Mission (XRISM). XRISM is scheduled to be launched in the Japanese fiscal year 2022. Xtend consists of the Soft X-ray Imager (SXI), an X-ray CCD camera, and the X-ray Mirror Assembly (XMA), a thin-foil-nested conically approximated Wolter-I optics. The SXI uses the P-channel, back-illuminated type CCD with an imaging area size of 31 mm on a side. The four CCD chips are arranged in a 2$\times$2 grid and can be cooled down to $-120$ $^{\circ}$C with a single-stage Stirling cooler. The XMA nests thin aluminum foils coated with gold in a confocal way with an outer diameter of 45~cm. A pre-collimator is installed in front of the X-ray mirror for the reduction of the stray light. Combining the SXI and XMA with a focal length of 5.6m, a field of view of $38^{\prime}\times38^{\prime}$ over the energy range from 0.4 to 13 keV is realized. We have completed the fabrication of the flight model of both SXI and XMA. The performance verification has been successfully conducted in a series of sub-system level tests. We also carried out on-ground calibration measurements and the data analysis is ongoing.<br />Comment: 11 pages, 13 figures. Proceedings of SPIE Astronomical Telescopes and Instrumentation 2022

Details

Database :
arXiv
Journal :
Proc. of SPIE vol. 12181, 121811T (2022)
Publication Type :
Report
Accession number :
edsarx.2303.07575
Document Type :
Working Paper
Full Text :
https://doi.org/10.1117/12.2626894