Koji Mori, Takeshi Go Tsuru, Kazuhiro Nakazawa, Y. Ueda, Shin Watanabe, Takaaki Tanaka, M. Ishida, Hironori Matsumoto, Hisamitsu Awaki, Hiroshi Murakami, Masayoshi Nobukawa, Ayaki Takeda, Yasushi Fukazawa, Hiroshi Tsunemi, Tadayuki Takahashi, A. E. Hornschemeier, Takashi Okajima, William W. Zhang, Brian J. Williams, Tonia M. Venters, Kristin K. Madsen, Mihoko Yukita, Hiroki Akamatsu, Aya Bamba, Teruaki Enoto, Yutaka Fujita, Akihiro Furuzawa, Kouichi Hagino, Kosei Ishimura, Masayuki Itoh, Tetsu Kitayama, Shōgo Kobayashi, Takayoshi Kohmura, Aya Kubota, Misaki Mizumoto, Tsunefumi Mizuno, Hiroshi Nakajima, Kumiko Nobukawa, Hirofumi Noda, Hirokazu Odaka, Naomi Ota, Toshiki Sato, M. Shidatsu, Hiromasa Suzuki, H. Takahashi, A. Tanimoto, Y. Terada, Yuichi Terashima, Hiroyuki Uchida, Y. Uchiyama, Hiroya Yamaguchi, Yoichi Yatsu

doi:10.1117/12.2628772

A broadband x-ray imaging spectroscopy in the 2030s: the FORCE mission

Koji Mori, Takeshi Go Tsuru, Kazuhiro Nakazawa, Y. Ueda, Shin Watanabe, Takaaki Tanaka, M. Ishida, Hironori Matsumoto, Hisamitsu Awaki, Hiroshi Murakami, Masayoshi Nobukawa, Ayaki Takeda, Yasushi Fukazawa, Hiroshi Tsunemi, Tadayuki Takahashi, A. E. Hornschemeier, Takashi Okajima, William W. Zhang, Brian J. Williams, Tonia M. Venters, Kristin K. Madsen, Mihoko Yukita, Hiroki Akamatsu, Aya Bamba, Teruaki Enoto, Yutaka Fujita, Akihiro Furuzawa, Kouichi Hagino, Kosei Ishimura, Masayuki Itoh, Tetsu Kitayama, Shōgo Kobayashi, Takayoshi Kohmura, Aya Kubota, Misaki Mizumoto, Tsunefumi Mizuno, Hiroshi Nakajima, Kumiko Nobukawa, Hirofumi Noda, Hirokazu Odaka, Naomi Ota, Toshiki Sato, M. Shidatsu, Hiromasa Suzuki, H. Takahashi, A. Tanimoto, Y. Terada, Yuichi Terashima, Hiroyuki Uchida, Y. Uchiyama, Hiroya Yamaguchi, Yoichi Yatsu

Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray · 2022

Read source ↗ All evidence

Summary

In this multi-messenger astronomy era, all the observational probes are improving their sensitivities and overall performance. The Focusing on Relativistic universe and Cosmic Evolution (FORCE) mission, the product of a JAXA/NASA collaboration, will reach a 10 times higher sensitivity in the hard X-ray band (E > 10 keV) in comparison with any previous hard x-ray missions, and provide simultaneous soft x-ray coverage. FORCE aims to be launched in the early 2030s, providing a perfect hard x-ray complement to the ESA flagship mission Athena. FORCE will be the most powerful x-ray probe for discovering obscured/hidden black holes and studying high energy particle acceleration in our Universe and will address how relativistic processes in the universe are realized and how these affect cosmic

Source type: Peer-reviewed study
DOI: 10.1117/12.2628772
Catalogue ID: SNmoic25z7-868bab

Pulse AI · ask about this record

Dig deeper with Pulse AI.

Pulse AI has read the whole catalogue. Ask about this record, its theme, or how the findings apply to UK farming and policy — every answer cites the underlying studies.

How does this finding apply in a UK context?→What are the most cited records on this topic?→