X-ray Performance of Back-Side Illuminated Type of Kyoto's X-ray Astronomical SOI Pixel Sensor, XRPIX

Makoto Itou; Takeshi Go Tsuru; Takaaki Tanaka; Ayaki Takeda; Hideaki Matsumura; Shunichi Ohmura; Shinya Nakashima; Yasuo Arai; Koji Mori; Ryota Takenaka; Yusuke Nishioka; Takayoshi Kohmura; Koki Tamasawa; Craig Tindall

arXiv · 1604.00170

X-ray Performance of Back-Side Illuminated Type of Kyoto's X-ray Astronomical SOI Pixel Sensor, XRPIX

Makoto Itou·Takeshi Go Tsuru·Takaaki Tanaka·Ayaki Takeda·Hideaki Matsumura·Shunichi Ohmura·Shinya Nakashima·Yasuo Arai·Koji Mori·Ryota Takenaka·Yusuke Nishioka·Takayoshi Kohmura·Koki Tamasawa·Craig Tindall

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Abstract

We have been developing X-ray SOI pixel Sensors, called "XRPIX", for future X-ray astronomy satellites that enable us to observe in the wide energy band of 0.5-40 keV. Since XRPIXs have the circuitry layer with a thickness of about 8 {\mu}m in the front side of the sensor, it is impossible to detect low energy X-rays with a front-illuminated type. So, we have been developing back-illuminated type of XRPIX with a less 1 {\mu}m dead layer in the back-side, which enables the sensitivity to reach 0.5 keV. We produced two types of back-side illuminated (BI) XRPIXs, one of which is produced in "Pizza process" which LBNL developed and the other is processed in the ion implantation and laser annealing. We irradiated both of the BI-XRPIXs with soft X-ray and investigate soft X-ray performance of them. We report results from soft X-ray evaluation test of the device.

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Makoto Itou, Takeshi Go Tsuru, Takaaki Tanaka, Ayaki Takeda, Hideaki Matsumura, Shunichi Ohmura, Shinya Nakashima, Yasuo Arai, Koji Mori, Ryota Takenaka, Yusuke Nishioka, Takayoshi Kohmura, Koki Tamasawa, Craig Tindall. 2016-04-01. X-ray Performance of Back-Side Illuminated Type of Kyoto's X-ray Astronomical SOI Pixel Sensor, XRPIX. https://arxiv.org/abs/1604.00170

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