The FORCE mission : Science aim and instrument parameter for broadband X-ray imaging spectroscopy with good angular resolution
Abstract
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 half-power-diameter. It is proposed to be launched around mid-2020s and designed to reach a limiting sensitivity as good as ~erg cm s keV within 1~Ms. This number is one order of magnitude better than current best one. With its high-sensitivity wide-band 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 large soft x-ray observatories.
Keywords
Cite
@article{arxiv.1807.11175,
title = {The FORCE mission : Science aim and instrument parameter for broadband X-ray imaging spectroscopy with good angular resolution},
author = {Kazuhiro Nakazawa and Koji Mori and Takeshi G. Tsuru and Yoshihiro Ueda and Hisamitsu Awaki and Yasushi Fukazawa and Manabu Ishida and Hironori Matsumoto and Hiroshi Murakami and Takashi Okajima and Tadayuki Takahashi and Hiroshi Tsunemi and William W. Zhang},
journal= {arXiv preprint arXiv:1807.11175},
year = {2018}
}
Comments
On SPIE Space Telescopes and Instrumentation 2018:Ultraviolet to Gamma Ray. 14 Pages, and 4 Figures