Development of four-stage x-ray telescope for DIOS (diffuse intergalactic oxygen surveyor) mission

Yuzuru Tawara; Akihiro Furuzawa; Yasushi Ogasaka; Keisuke Tamura; Takuya Miyazawa; Machiko Sakashita; Rika Takahashi

doi:10.1117/12.550881

Development of four-stage x-ray telescope for DIOS (diffuse intergalactic oxygen surveyor) mission

Yuzuru Tawara, Akihiro Furuzawa, Yasushi Ogasaka, Keisuke Tamura, Takuya Miyazawa, Machiko Sakashita, Rika Takahashi

Research output: Contribution to journal › Conference article

5 Citations (Scopus)

Abstract

Observation of diffuse soft X-rays with very low surface brightness can provide us cosmologically important information which is related to the missing baryon problem, large scale structure, etc. Diffuse Intergalactic Oxygen Surveyor(DIOS) mission is planned to observe such source, which may be originated by Warm Hot Intergalactic Medium( WHIM). For this purpose, the X-ray optical system designed under the condition of limited resource of the satellite, such as weight and size. Remarkable characteristic of this system is using four time reflection to fit their observational instrument to the small satellite. Numerical simulations were performed to evaluate X-ray observational performance such as grasp, angular resolution, field of view. In addition to the promissing way of mirror fabrication, aluminum foil based epoxy replication method, it will also be desribed that the present status of four-stage full shell mirror development.

Original language	English
Pages (from-to)	750-754
Number of pages	5
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	5488
Issue number	PART 2
DOIs	https://doi.org/10.1117/12.550881
Publication status	Published - 20-12-2004
Externally published	Yes
Event	UV and Gamma-Ray Space Telescope Systems - Glasgow, United Kingdom Duration: 21-06-2004 → 24-06-2004

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All Science Journal Classification (ASJC) codes

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

Cite this

Tawara, Y., Furuzawa, A., Ogasaka, Y., Tamura, K., Miyazawa, T., Sakashita, M., & Takahashi, R. (2004). Development of four-stage x-ray telescope for DIOS (diffuse intergalactic oxygen surveyor) mission. Proceedings of SPIE - The International Society for Optical Engineering, 5488(PART 2), 750-754. https://doi.org/10.1117/12.550881

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abstract = "Observation of diffuse soft X-rays with very low surface brightness can provide us cosmologically important information which is related to the missing baryon problem, large scale structure, etc. Diffuse Intergalactic Oxygen Surveyor(DIOS) mission is planned to observe such source, which may be originated by Warm Hot Intergalactic Medium( WHIM). For this purpose, the X-ray optical system designed under the condition of limited resource of the satellite, such as weight and size. Remarkable characteristic of this system is using four time reflection to fit their observational instrument to the small satellite. Numerical simulations were performed to evaluate X-ray observational performance such as grasp, angular resolution, field of view. In addition to the promissing way of mirror fabrication, aluminum foil based epoxy replication method, it will also be desribed that the present status of four-stage full shell mirror development.",

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Development of four-stage x-ray telescope for DIOS (diffuse intergalactic oxygen surveyor) mission. / Tawara, Yuzuru; Furuzawa, Akihiro; Ogasaka, Yasushi; Tamura, Keisuke; Miyazawa, Takuya; Sakashita, Machiko; Takahashi, Rika.

In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 5488, No. PART 2, 20.12.2004, p. 750-754.

Research output: Contribution to journal › Conference article

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AU - Tawara, Yuzuru

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AU - Miyazawa, Takuya

AU - Sakashita, Machiko

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10.1117/12.550881