Wide-band x-ray observatory for the time domain astronomy era: CHRONOS

Chronos is a X-ray observatory concept capable of “hour-level” follow up observations of transient alerts in 2030s’ multi-messenger astronomy, with 0.3–40+ keV wide X-ray band-width and 250–300 nm ultra-violet (UV) coverage. The mission has a good hard X-ray imaging spectroscopy with > 9′ field of view, the soft X-ray imager with > 30′ field of view, and the UV imager with > 7° field of view. Aiming at launch in mid-2030s, the mission is designed to provide wide-band spectroscopy of time dependent high-energy phenomena. The low background and large effective area in the hard X-ray band also make it good at observing diffuse hard X-ray emissions, such as many TeV sources which will be newly found in 2030s.

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Publication Details

Published
2024-08-21
DOI
https://doi.org/10.1117/12.3018366
Citations
1
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.33
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article

Wide-band x-ray observatory for the time domain astronomy era: CHRONOS

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article

Wide-band x-ray observatory for the time domain astronomy era: CHRONOS

M. Shidatsu, Mariko Kimura, T. Kawamuro, Hirofumi Noda, Y. Terada, Y. Ueda, Kosuke Namekata, Hiroyuki Uchida, Hiroya Yamaguchi, W. Iwakiri, Takaaki Tanaka, Takashi Okajima, Teruaki Enoto, Takeshi Go Tsuru, Hiroshi Nakajima, Kazuhiro Nakazawa, Masayoshi Nobukawa, H. Takahashi, Satoshi Yamada, Shin Watanabe, Koji Mori, Hironori Matsumoto, Hiromasa Suzuku, Hiroki Akamatsu, M. Ishida, Yoichi Yatsu
article en
1 citations

Abstract

Chronos is a X-ray observatory concept capable of “hour-level” follow up observations of transient alerts in 2030s’ multi-messenger astronomy, with 0.3–40+ keV wide X-ray band-width and 250–300 nm ultra-violet (UV) coverage. The mission has a good hard X-ray imaging spectroscopy with > 9′ field of view, the soft X-ray imager with > 30′ field of view, and the UV imager with > 7° field of view. Aiming at launch in mid-2030s, the mission is designed to provide wide-band spectroscopy of time dependent high-energy phenomena. The low background and large effective area in the hard X-ray band also make it good at observing diffuse hard X-ray emissions, such as many TeV sources which will be newly found in 2030s.

Kanazawa University (JP), Chiba University (JP), Kanto Gakuin University (JP), Kyoto University (JP), Japan Aerospace Exploration Agency (JP), Planetary Systems (United States) (US), Institute of Space and Astronautical Science (JP), Ehime University (JP), Nagoya University (JP)
Openalex Percentile: Top 35%
Astrophysical Phenomena and Observations
0.33
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