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Super DIOS Project for Exploring “Dark Baryon”

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Abstract

The Super DIOS project, which is an improved version of DIOS (Diffuse Intergalactic Oxygen Surveyor), is one of the candidates for Japan’s future scientific satellites, to be launched after 2030. The main scientific objective of the project is to unravel the flow of energy and metal cycles at various scales from galaxies, galaxy clusters to the warm-hot intergalactic medium along the Cosmic Web. The primary goal is the quantification of baryons, especially the unidentified “dark baryons”. Super DIOS will have a wide field of view of \(\sim\)1 degree, with an angular resolution of \(\sim\)15 arcseconds and high energy resolution (\(E/dE > 1000\)). The detector will be a 30 kilo-pixel array of Transition Edge sensor (TES) with a micro-wave SQUID multiplexer read-out system. In this paper, we report on the scientific concept of Super DIOS and the status of its newly developed technologies.

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Acknowledgements

We acknowledge support from all the members who supported the studies in the DIOS program. This project is partially supported by JSPS KAKENHI Grant Numbers 26220703, 15H05438, 17K05393, 18H01260, 20K20920, and 20H05857.

Author information

Authors and Affiliations

  1. Department of Physics, Saitama University, Saitama, Saitama, 338-8570, Japan

    K. Sato

  2. Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, 229-8510, Japan

    N. Y. Yamasaki, M. Ishida & Y. Maeda

  3. National Astronomical Observatory of Japan, Mitaka, Tokyo, 181-8588, Japan

    K. Mitsuda

  4. Department of Physics, Tokyo Metropolitan University, Hachioji, Tokyo, 192-0397, Japan

    Y. Ishisaki, Y. Fujita & Y. Ezoe

  5. Department of Physics, Nagoya University, Nagoya, Aichi, 464-8602, Japan

    I. Mitsuishi & Y. Tawara

  6. Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa Oiwakecho, Sakyo-ku, Kyoto, 606-8502, Japan

    K. Osato

  7. Department of Physics, Tokyo Institute of Technology, Meguro-ku, Tokyo, 152-8551, Japan

    N. Kawai

  8. Department of Physics, Tokyo University of Science, Shinjyuku-ku, Tokyo, 162-8601, Japan

    K. Matsushita

  9. Department of Physics, Yale University, New Haven, CT 06520, USA

    D. Nagai

  10. Center for Computational Sciences, University of Tsukuba, Tsukuba, 305-8571, Ibaraki, Japan

    K. Yoshikawa

  11. Faculty of Mathematics and Physics, Kanazawa University, Kanazawa, Ishikawa, 920-1192, Japan

    R. Fujimoto

  12. Department of Physics, Kyoto University, Sakyo-ku, Kyoto, 606-8502, Japan

    T. G. Tsuru

  13. Department of Physics, Nara Women’s University, Nara, Nara, 630-8506, Japan

    N. Ota

  14. Department of Physics, Rikkyo University, Toshima-Ku, Tokyo, 171-8501, Japan

    S. Yamada & Y. Ichinohe

  15. School of Science, Hiroshima University, Higashi-Hiroshima, Hiroshima, 739-8526, Japan

    Y. Uchida

  16. National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba, Ibaraki, 305-8568, Japan

    Y. Nakashima

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  1. K. Sato
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Correspondence to K. Sato.

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Sato, K., Yamasaki, N.Y., Ishida, M. et al. Super DIOS Project for Exploring “Dark Baryon”. J Low Temp Phys 209, 971–979 (2022). https://doi.org/10.1007/s10909-022-02910-w

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