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Future Japanese missions for the study of warm-hot intergalactic medium

T. Ohashi·M. Ishida·S. Sasaki·Y. Ishisaki·K. Mitsuda·N. Y. Yamasaki·R. Fujimoto·T. Furusho·H. Kunieda·Y. Tawara·A. Furuzawa·Y. Suto·K. Yoshikawa
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Abstract

We present our proposal for a small X-ray mission DIOS (Diffuse Intergalactic Oxygen Surveyor) to perform survey observations of warm-hot intergalactic medium using OVII and OVIII emission lines. This will be proposed to a small satellite program planned by ISAS/JAXA in Japan for a launch in 2008. The instrument consists of an array of TES microcalorimeters with an energy resolution 2 eV, cooled by mechanical coolers. The X-ray telescope will employ 4-stage reflection mirrors with a focal length as short as 70 cm and an angular resolution 2'. In addition to DIOS, we briefly describe the NeXT (New X-ray Telescope) mission, which is a larger Japanese X-ray observatory to be launched in 2010 and plans to explore non-thermal processes in the universe.

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T. Ohashi, M. Ishida, S. Sasaki, Y. Ishisaki, K. Mitsuda, N. Y. Yamasaki, R. Fujimoto, T. Furusho, H. Kunieda, Y. Tawara, A. Furuzawa, Y. Suto, K. Yoshikawa. 2004-02-24. Future Japanese missions for the study of warm-hot intergalactic medium. https://arxiv.org/abs/astro-ph/0402546

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