Pulse Brain · Growing Health Evidence Index
Peer-reviewed

The FORCE mission: science aim and instrument parameter for broadband x-ray imaging spectroscopy with good angular resolution

Koji Mori, Takeshi G. Tsuru, Yoshihiro Ueda, Hisamitsu Awaki, Yasushi Fukazawa, Manabu Ishida, Hironori Matsumoto, Hiroshi Murakami, Takashi Okajima, Hiroshi Tsunemi, William W. Zhang, Kazuhiro Nakazawa, Tadayuki Takahashi

Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray · 2018

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Summary

FORCE is a 1.2 tonnes small mission dedicated for wide-band fine-imaging x-ray observation. It covers from 1 to 80 keV with a good angular resolution of 15′′ half-power-diameter. It is proposed to be launched around mid2020s and designed to reach a limiting sensitivity as good as F<sub>X</sub>(10 − 40 keV) = 3 &times; 10<sup>−15</sup> erg cm<sup>−2</sup> s<sup> −1</sup> keV<sup>−1</sup> within 1 Ms. This number is one order of magnitude better than current best one. With its high-sensitivity wideband coverage, FORCE will probe the new science field of “missing BHs”, searching for families of black holes of which populations and evolutions are not well known. Other point-source and diffuse-source sciences are also considered. FORCE will also provide the “hard x-ray coverage” to forthcoming

Source type
Peer-reviewed study
DOI
10.1117/12.2309344
Catalogue ID
SNmoic25z7-3ppfs0
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