Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H

Kazuhisa Mitsuda; Richard L. Kelley; Hiroki Akamatsu; Thomas Bialas; Kevin R. Boyce; Gregory V. Brown; Edgar Canavan; Meng Chiao; Elisa Costantini; Jan Willem Den Herder; Cor De Vries; Michael J. Dipirro; Megan E. Eckart; Yuichiro Ezoe; Ryuichi Fujimoto; Daniel Haas; Akio Hoshino; Kumi Ishikawa; Yoshitaka Ishisaki; Naoko Iyomoto; Caroline A. Kilbourne; Mark Kimball; Shunji Kitamoto; Saori Konami; Maurice A. Leutenegger; Dan McCammon; Joseph Miko; Ikuyuki Mitsuishi; Hiroshi Murakami; Masahide Murakami; Hirofumi Noda; Mina Ogawa; Takaya Ohashi; Atsushi Okamoto; Naomi Ota; Stéphane Paltani; F. Scott Porter; Kosuke Sato; Yoichi Sato; Makoto Sawada; Hiromi Seta; Keisuke Shinozaki; Peter J. Shirron; Gary A. Sneiderman; Hiroyuki Sugita; Andrew Szymkowiak; Yoh Takei; Toru Tamagawa; Makoto S. Tashiro; Yukikatsu Terada; Masahiro Tsujimoto; Shinya Yamada; Noriko Y. Yamasaki

doi:10.1117/12.2057199

Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H

Kazuhisa Mitsuda, Richard L. Kelley, Hiroki Akamatsu, Thomas Bialas, Kevin R. Boyce, Gregory V. Brown, Edgar Canavan, Meng Chiao, Elisa Costantini, Jan Willem Den Herder, Cor De Vries, Michael J. Dipirro, Megan E. Eckart, Yuichiro Ezoe, Ryuichi Fujimoto, Daniel Haas, Akio Hoshino, Kumi Ishikawa, Yoshitaka Ishisaki, Naoko IyomotoCaroline A. Kilbourne, Mark Kimball, Shunji Kitamoto, Saori Konami, Maurice A. Leutenegger, Dan McCammon, Joseph Miko, Ikuyuki Mitsuishi, Hiroshi Murakami, Masahide Murakami, Hirofumi Noda, Mina Ogawa, Takaya Ohashi, Atsushi Okamoto, Naomi Ota, Stéphane Paltani, F. Scott Porter, Kosuke Sato, Yoichi Sato, Makoto Sawada, Hiromi Seta, Keisuke Shinozaki, Peter J. Shirron, Gary A. Sneiderman, Hiroyuki Sugita, Andrew Szymkowiak, Yoh Takei, Toru Tamagawa, Makoto S. Tashiro, Yukikatsu Terada, Masahiro Tsujimoto, Shinya Yamada, Noriko Y. Yamasaki

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

56 Citations (Scopus)

Abstract

We present the development status of the Soft X-ray Spectrometer (SXS) onboard the ASTRO-H mission. The SXS provides the capability of high energy-resolution X-ray spectroscopy of a FWHM energy resolution of < 7eV in the energy range of 0.3 - 10 keV. It utilizes an X-ray micorcalorimeter array operated at 50 mK. The SXS microcalorimeter subsystem is being developed in an EM-FM approach. The EM SXS cryostat was developed and fully tested and, although the design was generally confirmed, several anomalies and problems were found. Among them is the interference of the detector with the micro-vibrations from the mechanical coolers, which is the most difficult one to solve. We have pursued three different countermeasures and two of them seem to be effective. So far we have obtained energy resolutions satisfying the requirement with the FM cryostat.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2014
Subtitle of host publication	Ultraviolet to Gamma Ray
Editors	Tadayuki Takahashi, Jan-Willem A. den Herder, Mark Bautz
Publisher	SPIE
ISBN (Electronic)	9780819496126
DOIs	https://doi.org/10.1117/12.2057199
Publication status	Published - 2014
Externally published	Yes
Event	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray - Montreal, Canada Duration: 2014 Jun 22 → 2014 Jun 26

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9144
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Country/Territory	Canada
City	Montreal
Period	14/6/22 → 14/6/26

Keywords

High resolution X-ray Spectroscopy
Soft X-ray
X-ray astronomy

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2057199

Cite this

Mitsuda, K., Kelley, R. L., Akamatsu, H., Bialas, T., Boyce, K. R., Brown, G. V., Canavan, E., Chiao, M., Costantini, E., Den Herder, J. W., De Vries, C., Dipirro, M. J., Eckart, M. E., Ezoe, Y., Fujimoto, R., Haas, D., Hoshino, A., Ishikawa, K., Ishisaki, Y., ... Yamasaki, N. Y. (2014). Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H. In T. Takahashi, J-W. A. den Herder, & M. Bautz (Eds.), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray [91442A] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9144). SPIE. https://doi.org/10.1117/12.2057199

Soft x-ray spectrometer (SXS) : The high-resolution cryogenic spectrometer onboard ASTRO-H. / Mitsuda, Kazuhisa; Kelley, Richard L.; Akamatsu, Hiroki et al.

Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. ed. / Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz. SPIE, 2014. 91442A (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9144).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Mitsuda, K, Kelley, RL, Akamatsu, H, Bialas, T, Boyce, KR, Brown, GV, Canavan, E, Chiao, M, Costantini, E, Den Herder, JW, De Vries, C, Dipirro, MJ, Eckart, ME, Ezoe, Y, Fujimoto, R, Haas, D, Hoshino, A, Ishikawa, K, Ishisaki, Y, Iyomoto, N, Kilbourne, CA, Kimball, M, Kitamoto, S, Konami, S, Leutenegger, MA, McCammon, D, Miko, J, Mitsuishi, I, Murakami, H, Murakami, M, Noda, H, Ogawa, M, Ohashi, T, Okamoto, A, Ota, N, Paltani, S, Porter, FS, Sato, K, Sato, Y, Sawada, M, Seta, H, Shinozaki, K, Shirron, PJ, Sneiderman, GA, Sugita, H, Szymkowiak, A, Takei, Y, Tamagawa, T, Tashiro, MS, Terada, Y, Tsujimoto, M, Yamada, S & Yamasaki, NY 2014, Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H. in T Takahashi, J-WA den Herder & M Bautz (eds), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray., 91442A, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9144, SPIE, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, Montreal, Canada, 14/6/22. https://doi.org/10.1117/12.2057199

Mitsuda K, Kelley RL, Akamatsu H, Bialas T, Boyce KR, Brown GV et al. Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H. In Takahashi T, den Herder J-WA, Bautz M, editors, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. SPIE. 2014. 91442A. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2057199

Mitsuda, Kazuhisa ; Kelley, Richard L. ; Akamatsu, Hiroki et al. / Soft x-ray spectrometer (SXS) : The high-resolution cryogenic spectrometer onboard ASTRO-H. Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. editor / Tadayuki Takahashi ; Jan-Willem A. den Herder ; Mark Bautz. SPIE, 2014. (Proceedings of SPIE - The International Society for Optical Engineering).

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title = "Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H",

abstract = "We present the development status of the Soft X-ray Spectrometer (SXS) onboard the ASTRO-H mission. The SXS provides the capability of high energy-resolution X-ray spectroscopy of a FWHM energy resolution of < 7eV in the energy range of 0.3 - 10 keV. It utilizes an X-ray micorcalorimeter array operated at 50 mK. The SXS microcalorimeter subsystem is being developed in an EM-FM approach. The EM SXS cryostat was developed and fully tested and, although the design was generally confirmed, several anomalies and problems were found. Among them is the interference of the detector with the micro-vibrations from the mechanical coolers, which is the most difficult one to solve. We have pursued three different countermeasures and two of them seem to be effective. So far we have obtained energy resolutions satisfying the requirement with the FM cryostat.",

keywords = "High resolution X-ray Spectroscopy, Soft X-ray, X-ray astronomy",

author = "Kazuhisa Mitsuda and Kelley, {Richard L.} and Hiroki Akamatsu and Thomas Bialas and Boyce, {Kevin R.} and Brown, {Gregory V.} and Edgar Canavan and Meng Chiao and Elisa Costantini and {Den Herder}, {Jan Willem} and {De Vries}, Cor and Dipirro, {Michael J.} and Eckart, {Megan E.} and Yuichiro Ezoe and Ryuichi Fujimoto and Daniel Haas and Akio Hoshino and Kumi Ishikawa and Yoshitaka Ishisaki and Naoko Iyomoto and Kilbourne, {Caroline A.} and Mark Kimball and Shunji Kitamoto and Saori Konami and Leutenegger, {Maurice A.} and Dan McCammon and Joseph Miko and Ikuyuki Mitsuishi and Hiroshi Murakami and Masahide Murakami and Hirofumi Noda and Mina Ogawa and Takaya Ohashi and Atsushi Okamoto and Naomi Ota and St{\'e}phane Paltani and Porter, {F. Scott} and Kosuke Sato and Yoichi Sato and Makoto Sawada and Hiromi Seta and Keisuke Shinozaki and Shirron, {Peter J.} and Sneiderman, {Gary A.} and Hiroyuki Sugita and Andrew Szymkowiak and Yoh Takei and Toru Tamagawa and Tashiro, {Makoto S.} and Yukikatsu Terada and Masahiro Tsujimoto and Shinya Yamada and Yamasaki, {Noriko Y.}",

note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray ; Conference date: 22-06-2014 Through 26-06-2014",

year = "2014",

doi = "10.1117/12.2057199",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Tadayuki Takahashi and {den Herder}, {Jan-Willem A.} and Mark Bautz",

booktitle = "Space Telescopes and Instrumentation 2014",

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T2 - Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray

AU - Mitsuda, Kazuhisa

AU - Kelley, Richard L.

AU - Akamatsu, Hiroki

AU - Bialas, Thomas

AU - Boyce, Kevin R.

AU - Brown, Gregory V.

AU - Canavan, Edgar

AU - Chiao, Meng

AU - Costantini, Elisa

AU - Den Herder, Jan Willem

AU - De Vries, Cor

AU - Dipirro, Michael J.

AU - Eckart, Megan E.

AU - Ezoe, Yuichiro

AU - Fujimoto, Ryuichi

AU - Haas, Daniel

AU - Hoshino, Akio

AU - Ishikawa, Kumi

AU - Ishisaki, Yoshitaka

AU - Iyomoto, Naoko

AU - Kilbourne, Caroline A.

AU - Kimball, Mark

AU - Kitamoto, Shunji

AU - Konami, Saori

AU - Leutenegger, Maurice A.

AU - McCammon, Dan

AU - Miko, Joseph

AU - Mitsuishi, Ikuyuki

AU - Murakami, Hiroshi

AU - Murakami, Masahide

AU - Noda, Hirofumi

AU - Ogawa, Mina

AU - Ohashi, Takaya

AU - Okamoto, Atsushi

AU - Ota, Naomi

AU - Paltani, Stéphane

AU - Porter, F. Scott

AU - Sato, Kosuke

AU - Sato, Yoichi

AU - Sawada, Makoto

AU - Seta, Hiromi

AU - Shinozaki, Keisuke

AU - Shirron, Peter J.

AU - Sneiderman, Gary A.

AU - Sugita, Hiroyuki

AU - Szymkowiak, Andrew

AU - Takei, Yoh

AU - Tamagawa, Toru

AU - Tashiro, Makoto S.

AU - Terada, Yukikatsu

AU - Tsujimoto, Masahiro

AU - Yamada, Shinya

AU - Yamasaki, Noriko Y.

PY - 2014

Y1 - 2014

N2 - We present the development status of the Soft X-ray Spectrometer (SXS) onboard the ASTRO-H mission. The SXS provides the capability of high energy-resolution X-ray spectroscopy of a FWHM energy resolution of < 7eV in the energy range of 0.3 - 10 keV. It utilizes an X-ray micorcalorimeter array operated at 50 mK. The SXS microcalorimeter subsystem is being developed in an EM-FM approach. The EM SXS cryostat was developed and fully tested and, although the design was generally confirmed, several anomalies and problems were found. Among them is the interference of the detector with the micro-vibrations from the mechanical coolers, which is the most difficult one to solve. We have pursued three different countermeasures and two of them seem to be effective. So far we have obtained energy resolutions satisfying the requirement with the FM cryostat.

AB - We present the development status of the Soft X-ray Spectrometer (SXS) onboard the ASTRO-H mission. The SXS provides the capability of high energy-resolution X-ray spectroscopy of a FWHM energy resolution of < 7eV in the energy range of 0.3 - 10 keV. It utilizes an X-ray micorcalorimeter array operated at 50 mK. The SXS microcalorimeter subsystem is being developed in an EM-FM approach. The EM SXS cryostat was developed and fully tested and, although the design was generally confirmed, several anomalies and problems were found. Among them is the interference of the detector with the micro-vibrations from the mechanical coolers, which is the most difficult one to solve. We have pursued three different countermeasures and two of them seem to be effective. So far we have obtained energy resolutions satisfying the requirement with the FM cryostat.

KW - High resolution X-ray Spectroscopy

KW - Soft X-ray

KW - X-ray astronomy

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U2 - 10.1117/12.2057199

DO - 10.1117/12.2057199

M3 - Conference contribution

AN - SCOPUS:84922534341

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2014

A2 - Takahashi, Tadayuki

A2 - den Herder, Jan-Willem A.

A2 - Bautz, Mark

PB - SPIE

Y2 - 22 June 2014 through 26 June 2014

ER -

Soft x-ray spectrometer (SXS): The high-resolution cryogenic spectrometer onboard ASTRO-H

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

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