Status of Xtend telescope onboard X-Ray Imaging and Spectroscopy Mission (XRISM)

Fuente: arXiv
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Autori principali: Mori, Koji, Tomida, Hiroshi, Nakajima, Hiroshi, Okajima, Takashi, Noda, Hirofumi, Uchida, Hiroyuki, Suzuki, Hiromasa, Kobayashi, Shogo Benjamin, Yoneyama, Tomokage, Hagino, Kouichi, Nobukawa, Kumiko, Tanaka, Takaaki, Murakami, Hiroshi, Uchiyama, Hideki, Nobukawa, Masayoshi, Matsumoto, Hironori, Tsuru, Takeshi, Yamauchi, Makoto, Hatsukade, Isamu, Odaka, Hirokazu, Kohmura, Takayoshi, Yamaoka, Kazutaka, Ishida, Manabu, Maeda, Yoshitomo, Hayashi, Takayuki, Tamura, Keisuke, Boissay-Malaquin, Rozenn, Sato, Toshiki, Yoshida, Tessei, Kanemaru, Yoshiaki, Hiraga, Junko, Dotani, Tadayasu, Ozaki, Masanobu, Tsunemi, Hiroshi, Inoue, Shun, Azuma, Ryuishi, Aoki, Yuma, Asahina, Yoh, Nakamura, Shotaro, Kamei, Takamitsu, Fukuda, Masahiro, Asakura, Kazunori, Yoshimoto, Marina, Ode, Yuichi, Hakamata, Tomohiro, Aoyagi, Mio, shima, Kohei, Ito, Yamato, Aoki, Daiki, Fujisawa, Kaito, Shimizu, Yasuyuki, Higuchi, Mayu, Miyazaki, Keitaro, Kusunoki, Kohei, Otsuka, Yoshinori, Yokosu, Haruhiko, Yonemaru, Wakana, Ichikawa, Kazuhiro, Nakano, Hanako, takemoto, Reo, Matsushima, Tsukasa, Hayashida, Kiyoshi
Natura: Preprint
Pubblicazione: 2024
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author Mori, Koji
Tomida, Hiroshi
Nakajima, Hiroshi
Okajima, Takashi
Noda, Hirofumi
Uchida, Hiroyuki
Suzuki, Hiromasa
Kobayashi, Shogo Benjamin
Yoneyama, Tomokage
Hagino, Kouichi
Nobukawa, Kumiko
Tanaka, Takaaki
Murakami, Hiroshi
Uchiyama, Hideki
Nobukawa, Masayoshi
Matsumoto, Hironori
Tsuru, Takeshi
Yamauchi, Makoto
Hatsukade, Isamu
Odaka, Hirokazu
Kohmura, Takayoshi
Yamaoka, Kazutaka
Ishida, Manabu
Maeda, Yoshitomo
Hayashi, Takayuki
Tamura, Keisuke
Boissay-Malaquin, Rozenn
Sato, Toshiki
Yoshida, Tessei
Kanemaru, Yoshiaki
Hiraga, Junko
Dotani, Tadayasu
Ozaki, Masanobu
Tsunemi, Hiroshi
Inoue, Shun
Azuma, Ryuishi
Aoki, Yuma
Asahina, Yoh
Nakamura, Shotaro
Kamei, Takamitsu
Fukuda, Masahiro
Asakura, Kazunori
Yoshimoto, Marina
Ode, Yuichi
Hakamata, Tomohiro
Aoyagi, Mio
shima, Kohei
Aoki, Yuma
Ito, Yamato
Aoki, Daiki
Fujisawa, Kaito
Shimizu, Yasuyuki
Higuchi, Mayu
Miyazaki, Keitaro
Kusunoki, Kohei
Otsuka, Yoshinori
Yokosu, Haruhiko
Yonemaru, Wakana
Ichikawa, Kazuhiro
Nakano, Hanako
takemoto, Reo
Matsushima, Tsukasa
Hayashida, Kiyoshi
author_facet Mori, Koji
Tomida, Hiroshi
Nakajima, Hiroshi
Okajima, Takashi
Noda, Hirofumi
Uchida, Hiroyuki
Suzuki, Hiromasa
Kobayashi, Shogo Benjamin
Yoneyama, Tomokage
Hagino, Kouichi
Nobukawa, Kumiko
Tanaka, Takaaki
Murakami, Hiroshi
Uchiyama, Hideki
Nobukawa, Masayoshi
Matsumoto, Hironori
Tsuru, Takeshi
Yamauchi, Makoto
Hatsukade, Isamu
Odaka, Hirokazu
Kohmura, Takayoshi
Yamaoka, Kazutaka
Ishida, Manabu
Maeda, Yoshitomo
Hayashi, Takayuki
Tamura, Keisuke
Boissay-Malaquin, Rozenn
Sato, Toshiki
Yoshida, Tessei
Kanemaru, Yoshiaki
Hiraga, Junko
Dotani, Tadayasu
Ozaki, Masanobu
Tsunemi, Hiroshi
Inoue, Shun
Azuma, Ryuishi
Aoki, Yuma
Asahina, Yoh
Nakamura, Shotaro
Kamei, Takamitsu
Fukuda, Masahiro
Asakura, Kazunori
Yoshimoto, Marina
Ode, Yuichi
Hakamata, Tomohiro
Aoyagi, Mio
shima, Kohei
Aoki, Yuma
Ito, Yamato
Aoki, Daiki
Fujisawa, Kaito
Shimizu, Yasuyuki
Higuchi, Mayu
Miyazaki, Keitaro
Kusunoki, Kohei
Otsuka, Yoshinori
Yokosu, Haruhiko
Yonemaru, Wakana
Ichikawa, Kazuhiro
Nakano, Hanako
takemoto, Reo
Matsushima, Tsukasa
Hayashida, Kiyoshi
contents Xtend is one of the two telescopes onboard the X-ray imaging and spectroscopy mission (XRISM), which was launched on September 7th, 2023. Xtend comprises 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. A large field of view of $38^{\prime}\times38^{\prime}$ over the energy range from 0.4 to 13 keV is realized by the combination of the SXI and XMA with a focal length of 5.6 m. The SXI employs four P-channel, back-illuminated type CCDs with a thick depletion layer of 200 $μ$m. The four CCD chips are arranged in a 2$\times$2 grid and cooled down to $-110$ $^{\circ}$C with a single-stage Stirling cooler. Before the launch of XRISM, we conducted a month-long spacecraft thermal vacuum test. The performance verification of the SXI was successfully carried out in a course of multiple thermal cycles of the spacecraft. About a month after the launch of XRISM, the SXI was carefully activated and the soundness of its functionality was checked by a step-by-step process. Commissioning observations followed the initial operation. We here present pre- and post-launch results verifying the Xtend performance. All the in-orbit performances are consistent with those measured on ground and satisfy the mission requirement. Extensive calibration studies are ongoing.
format Preprint
id arxiv_https___arxiv_org_abs_2406_19911
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Status of Xtend telescope onboard X-Ray Imaging and Spectroscopy Mission (XRISM)
Mori, Koji
Tomida, Hiroshi
Nakajima, Hiroshi
Okajima, Takashi
Noda, Hirofumi
Uchida, Hiroyuki
Suzuki, Hiromasa
Kobayashi, Shogo Benjamin
Yoneyama, Tomokage
Hagino, Kouichi
Nobukawa, Kumiko
Tanaka, Takaaki
Murakami, Hiroshi
Uchiyama, Hideki
Nobukawa, Masayoshi
Matsumoto, Hironori
Tsuru, Takeshi
Yamauchi, Makoto
Hatsukade, Isamu
Odaka, Hirokazu
Kohmura, Takayoshi
Yamaoka, Kazutaka
Ishida, Manabu
Maeda, Yoshitomo
Hayashi, Takayuki
Tamura, Keisuke
Boissay-Malaquin, Rozenn
Sato, Toshiki
Yoshida, Tessei
Kanemaru, Yoshiaki
Hiraga, Junko
Dotani, Tadayasu
Ozaki, Masanobu
Tsunemi, Hiroshi
Inoue, Shun
Azuma, Ryuishi
Aoki, Yuma
Asahina, Yoh
Nakamura, Shotaro
Kamei, Takamitsu
Fukuda, Masahiro
Asakura, Kazunori
Yoshimoto, Marina
Ode, Yuichi
Hakamata, Tomohiro
Aoyagi, Mio
shima, Kohei
Aoki, Yuma
Ito, Yamato
Aoki, Daiki
Fujisawa, Kaito
Shimizu, Yasuyuki
Higuchi, Mayu
Miyazaki, Keitaro
Kusunoki, Kohei
Otsuka, Yoshinori
Yokosu, Haruhiko
Yonemaru, Wakana
Ichikawa, Kazuhiro
Nakano, Hanako
takemoto, Reo
Matsushima, Tsukasa
Hayashida, Kiyoshi
Instrumentation and Methods for Astrophysics
Xtend is one of the two telescopes onboard the X-ray imaging and spectroscopy mission (XRISM), which was launched on September 7th, 2023. Xtend comprises 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. A large field of view of $38^{\prime}\times38^{\prime}$ over the energy range from 0.4 to 13 keV is realized by the combination of the SXI and XMA with a focal length of 5.6 m. The SXI employs four P-channel, back-illuminated type CCDs with a thick depletion layer of 200 $μ$m. The four CCD chips are arranged in a 2$\times$2 grid and cooled down to $-110$ $^{\circ}$C with a single-stage Stirling cooler. Before the launch of XRISM, we conducted a month-long spacecraft thermal vacuum test. The performance verification of the SXI was successfully carried out in a course of multiple thermal cycles of the spacecraft. About a month after the launch of XRISM, the SXI was carefully activated and the soundness of its functionality was checked by a step-by-step process. Commissioning observations followed the initial operation. We here present pre- and post-launch results verifying the Xtend performance. All the in-orbit performances are consistent with those measured on ground and satisfy the mission requirement. Extensive calibration studies are ongoing.
title Status of Xtend telescope onboard X-Ray Imaging and Spectroscopy Mission (XRISM)
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2406.19911