Presentation
13 December 2020 The FORCE mission: focusing on relativistic universe and cosmic evolution
Author Affiliations +
Abstract
We present the concept of a future Japan-lead X-ray mission, FORCE (Focusing On Relativistic universe and Cosmic Evolution). FORCE is characterized by broadband (1-80 keV) X-ray imaging spectroscopy with high angular resolution (<15"). The sensitivity above 10 keV will be 10 times higher than that of any previous hard X-ray missions. FORCE will trace the cosmic evolution by searching for ``missing black holes'' in the entire range of their mass spectrum and investigate the nature of relativistic particles at various astrophysical shocks by observing their non-thermal X-ray emission.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Koji Mori, Takeshi G. Tsuru, Kazuhiro Nakazawa, Yoshihiro Ueda, Manabu Ishida, Takaaki Tanaka, Hironori Matsumoto, Hisamitsu Awaki, Hiroshi Murakami, Masayoshi Nobukawa, Ayaki Takeda, Shin Watanabe, Yasushi Fukazawa, Hiroshi Tsunemi, Tadayuki Takahashi, Ann E. Hornschemeier, Takashi Okajima, William W. Zhang, and Brian J. Williams "The FORCE mission: focusing on relativistic universe and cosmic evolution", Proc. SPIE 11444, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, 114442B (13 December 2020); https://doi.org/10.1117/12.2562151
Advertisement
Advertisement
KEYWORDS
X-rays

Atmospheric particles

Imaging spectroscopy

Spatial resolution

Spectroscopy

X-ray imaging

Active galactic nuclei

RELATED CONTENT

The ASTRO-H X-ray Observatory
Proceedings of SPIE (September 17 2012)
Future x-ray missions: the extragalactic perspective
Proceedings of SPIE (December 16 2002)
An overview of the IXO Observatory
Proceedings of SPIE (July 29 2010)

Back to Top