Status of the DIOS mission

Y. Tawara; I. Sakurai; A. Furuzawa; T. Ohashi; Y. Ishisaki; Y. Ezoe; A. Hoshino; H. Akamatsu; K. Ishikawa; K. Mitsuda; N. Y. Yamasaki; Y. Takei; K. Shinozaki; K. Masui; T. Yoshino; T. Hagihara; S. Kimura; H. Yoshitake

doi:10.1117/12.788144

Status of the DIOS mission

Y. Tawara, I. Sakurai, A. Furuzawa, T. Ohashi, Y. Ishisaki, Y. Ezoe, A. Hoshino, H. Akamatsu, K. Ishikawa, K. Mitsuda, N. Y. Yamasaki, Y. Takei, K. Shinozaki, K. Masui, T. Yoshino, T. Hagihara, S. Kimura, H. Yoshitake

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

11 Citations (Scopus)

Abstract

We present the current status of a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor), consisting of a 4-stage X-ray telescope and an array of TES microcalorimeters, cooled with mechanical coolers, with a total weight of about 400 kg. The mission will perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines, with the energy coverage up to 1.5 keV. The wide field of view of about 50′ diameter, superior energy resolution close to 2 eV FWHM, and very low background will together enable us a wide range of science for diffuse X-ray sources. We briefly describe the current status of the development of the satellite, and the subsystems.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2008
Subtitle of host publication	Ultraviolet to Gamma Ray
DOIs	https://doi.org/10.1117/12.788144
Publication status	Published - 2008
Externally published	Yes
Event	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille, France Duration: 23-06-2008 → 28-06-2008

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7011
ISSN (Print)	0277-786X

Other

Other	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
Country/Territory	France
City	Marseille
Period	23-06-08 → 28-06-08

All Science Journal Classification (ASJC) codes

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

Access to Document

10.1117/12.788144

Cite this

Tawara, Y., Sakurai, I., Furuzawa, A., Ohashi, T., Ishisaki, Y., Ezoe, Y., Hoshino, A., Akamatsu, H., Ishikawa, K., Mitsuda, K., Yamasaki, N. Y., Takei, Y., Shinozaki, K., Masui, K., Yoshino, T., Hagihara, T., Kimura, S., & Yoshitake, H. (2008). Status of the DIOS mission. In Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray Article 70111H (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7011). https://doi.org/10.1117/12.788144

@inproceedings{75eccb5a25014911934081ea9b22975c,

title = "Status of the DIOS mission",

abstract = "We present the current status of a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor), consisting of a 4-stage X-ray telescope and an array of TES microcalorimeters, cooled with mechanical coolers, with a total weight of about 400 kg. The mission will perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines, with the energy coverage up to 1.5 keV. The wide field of view of about 50′ diameter, superior energy resolution close to 2 eV FWHM, and very low background will together enable us a wide range of science for diffuse X-ray sources. We briefly describe the current status of the development of the satellite, and the subsystems.",

author = "Y. Tawara and I. Sakurai and A. Furuzawa and T. Ohashi and Y. Ishisaki and Y. Ezoe and A. Hoshino and H. Akamatsu and K. Ishikawa and K. Mitsuda and Yamasaki, {N. Y.} and Y. Takei and K. Shinozaki and K. Masui and T. Yoshino and T. Hagihara and S. Kimura and H. Yoshitake",

year = "2008",

doi = "10.1117/12.788144",

language = "English",

isbn = "9780819472212",

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

booktitle = "Space Telescopes and Instrumentation 2008",

note = "Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray ; Conference date: 23-06-2008 Through 28-06-2008",

}

Tawara, Y, Sakurai, I, Furuzawa, A, Ohashi, T, Ishisaki, Y, Ezoe, Y, Hoshino, A, Akamatsu, H, Ishikawa, K, Mitsuda, K, Yamasaki, NY, Takei, Y, Shinozaki, K, Masui, K, Yoshino, T, Hagihara, T, Kimura, S & Yoshitake, H 2008, Status of the DIOS mission. in Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray., 70111H, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, Marseille, France, 23-06-08. https://doi.org/10.1117/12.788144

TY - GEN

T1 - Status of the DIOS mission

AU - Tawara, Y.

AU - Sakurai, I.

AU - Furuzawa, A.

AU - Ohashi, T.

AU - Ishisaki, Y.

AU - Ezoe, Y.

AU - Hoshino, A.

AU - Akamatsu, H.

AU - Ishikawa, K.

AU - Mitsuda, K.

AU - Yamasaki, N. Y.

AU - Takei, Y.

AU - Shinozaki, K.

AU - Masui, K.

AU - Yoshino, T.

AU - Hagihara, T.

AU - Kimura, S.

AU - Yoshitake, H.

PY - 2008

Y1 - 2008

N2 - We present the current status of a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor), consisting of a 4-stage X-ray telescope and an array of TES microcalorimeters, cooled with mechanical coolers, with a total weight of about 400 kg. The mission will perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines, with the energy coverage up to 1.5 keV. The wide field of view of about 50′ diameter, superior energy resolution close to 2 eV FWHM, and very low background will together enable us a wide range of science for diffuse X-ray sources. We briefly describe the current status of the development of the satellite, and the subsystems.

AB - We present the current status of a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor), consisting of a 4-stage X-ray telescope and an array of TES microcalorimeters, cooled with mechanical coolers, with a total weight of about 400 kg. The mission will perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines, with the energy coverage up to 1.5 keV. The wide field of view of about 50′ diameter, superior energy resolution close to 2 eV FWHM, and very low background will together enable us a wide range of science for diffuse X-ray sources. We briefly describe the current status of the development of the satellite, and the subsystems.

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DO - 10.1117/12.788144

M3 - Conference contribution

AN - SCOPUS:70249127640

SN - 9780819472212

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

BT - Space Telescopes and Instrumentation 2008

T2 - Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray

Y2 - 23 June 2008 through 28 June 2008

ER -

Status of the DIOS mission

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