Kyoto's Event-Driven X-ray Astronomy SOI pixel sensor for the FORCE mission
Takeshi G. Tsuru, Hideki Hayashi, Katsuhiro Tachibana, Sodai Harada,, Hiroyuki Uchida, Takaaki Tanaka, Yasuo Arai, Ikuo Kurachi, Koji Mori, Ayaki, Takeda, Yusuke Nishioka, Nobuaki Takebayashi, Shoma Yokoyama, Kohei Fukuda,, Takayoshi Kohmura, Kouichi Hagino, Kenji Ohno

TL;DR
This paper reports on the development of advanced SOI pixel sensors for the FORCE X-ray astronomy mission, featuring high sensitivity, fast event-driven readout, and improved spectral performance through novel device structures.
Contribution
It introduces new monolithic SOI pixel sensors with enhanced imaging area, event-driven readout, and structural improvements for better spectral resolution and reduced noise.
Findings
Successful development of a large-area back-side illuminated device.
Double SOI structure improves spectral performance.
Pinned Depleted Diode structure reduces dark current and enhances energy resolution.
Abstract
We have been developing monolithic active pixel sensors, X-ray Astronomy SOI pixel sensors, XRPIXs, based on a Silicon-On-Insulator (SOI) CMOS technology as soft X-ray sensors for a future Japanese mission, FORCE (Focusing On Relativistic universe and Cosmic Evolution). The mission is characterized by broadband (1-80 keV) X-ray imaging spectroscopy with high angular resolution (~arcsec), with which we can achieve about ten times higher sensitivity in comparison to the previous missions above 10~keV. Immediate readout of only those pixels hit by an X-ray is available by an event trigger output function implemented in each pixel with the time resolution higher than (Event-Driven readout mode). It allows us to do fast timing observation and also reduces non-X-ray background dominating at a high X-ray energy band above 5--10~keV by adopting an anti-coincidence…
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