K. Mori, H. Tomida, H. Nakajima, T. Okajima, H. Noda, Takaaki Tanaka, H. Uchida, K. Hagino, S. Kobayashi, Hiromasa Suzuki, Tessei Yoshida, H. Murakami, H. Uchiyama, M. Nobukawa, K. Nobukawa, T. Yoneyama, H. Matsumoto, T. Tsuru, M. Yamauchi, I. Hatsukade, M. Ishida, Y. Maeda, T. Hayashi, K. Tamura, R. Boissay-Malaquin, Toshiki Sato, J. Hiraga, T. Kohmura, K. Yamaoka, T. Dotani, M. Ozaki, H. Tsunemi, Y. Kanemaru, J. Sato, Toshiyuki Takaki, Yuta Terada, Keitaro Miyazaki, Kohei Kusunoki, Y. Otsuka, Haruhiko Yokosu, Wakana Yonemaru, Yoh Asahina, K. Asakura, M. Yoshimoto, Yuichi Ode, J. Sato, T. Hakamata, Mio Aoyagi, Yuma Aoki, Shun Tsunomachi, T. Doi, D. Aoki, Kaito Fujisawa, Masatoshi Kitajima, K. Hayashida
{"title":"Xtend, the soft x-ray imaging telescope for the X-Ray Imaging and Spectroscopy Mission (XRISM)","authors":"K. Mori, H. Tomida, H. Nakajima, T. Okajima, H. Noda, Takaaki Tanaka, H. Uchida, K. Hagino, S. Kobayashi, Hiromasa Suzuki, Tessei Yoshida, H. Murakami, H. Uchiyama, M. Nobukawa, K. Nobukawa, T. Yoneyama, H. Matsumoto, T. Tsuru, M. Yamauchi, I. Hatsukade, M. Ishida, Y. Maeda, T. Hayashi, K. Tamura, R. Boissay-Malaquin, Toshiki Sato, J. Hiraga, T. Kohmura, K. Yamaoka, T. Dotani, M. Ozaki, H. Tsunemi, Y. Kanemaru, J. Sato, Toshiyuki Takaki, Yuta Terada, Keitaro Miyazaki, Kohei Kusunoki, Y. Otsuka, Haruhiko Yokosu, Wakana Yonemaru, Yoh Asahina, K. Asakura, M. Yoshimoto, Yuichi Ode, J. Sato, T. Hakamata, Mio Aoyagi, Yuma Aoki, Shun Tsunomachi, T. Doi, D. Aoki, Kaito Fujisawa, Masatoshi Kitajima, K. Hayashida","doi":"10.1117/12.2626894","DOIUrl":null,"url":null,"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 31mm on a side. The four CCD chips are arranged in a 2×2 grid and can be cooled down to −120 °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′ × 38′ 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.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2626894","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 4
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 31mm on a side. The four CCD chips are arranged in a 2×2 grid and can be cooled down to −120 °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′ × 38′ 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.