Low-energy X-ray performance of SOI pixel sensors for astronomy, “XRPIX”

We have been developing a new type of X-ray pixel sensors, "XRPIX", allowing us to perform imaging spectroscopy in the wide energy band of 1-20 keV for the future Japanese X-ray satellite "FORCE". The XRPIX devices are fabricated with complementary metal-oxide-semiconductor silicon-on-insulator technology, and have the "Event-Driven readout mode", in which only a hit event is read out by using hit information from a trigger output function equipped with each pixel. This paper reports on the low-energy X-ray performance of the "XRPIX6E" device with a Pinned Depleted Diode (PDD) structure. The PDD structure especially reduces the readout noise, and hence is expected to largely improve the quantum efficiencies for low-energy X-rays. While F-K X-rays at 0.68 keV and Al-K X-rays at 1.5 keV are successfully detected in the "Frame readout mode", in which all pixels are read out serially without using the trigger output function, the device is able to detect Al-K X-rays, but not F-K X-rays in the Event-Driven readout mode. Non-uniformity is observed in the counts maps of Al-K X-rays in the Event-Driven readout mode, which is due to region-to-region variation of the pedestal voltages at the input to the comparator circuit. The lowest available threshold energy is 1.1 keV for a small region in the device where the non-uniformity is minimized. The noise of the charge sensitive amplifier at the sense node and the noise related to the trigger output function are ~$18~e^-$ (rms) and ~$13~e^-$ (rms), respectively.

[1]  William W. Zhang,et al.  A broadband x-ray imaging spectroscopy with high-angular resolution: the FORCE mission , 2016, Astronomical Telescopes + Instrumentation.

[2]  Shoji Kawahito,et al.  Performance of the Silicon-On-Insulator pixel sensor for X-ray astronomy, XRPIX6E, equipped with pinned depleted diode structure , 2018, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment.

[3]  K. Hara,et al.  Development of SOI pixel process technology , 2011 .

[4]  Atsushi Iwata,et al.  First Performance Evaluation of an X-Ray SOI Pixel Sensor for Imaging Spectroscopy and Intra-Pixel Trigger , 2011, IEEE Transactions on Nuclear Science.

[5]  A. Mozzanica,et al.  Characterization and Calibration of PILATUS Detectors , 2009, IEEE Transactions on Nuclear Science.

[6]  Y. Arai,et al.  The first back-side illuminated types of Kyoto's X-ray astronomy SOIPIX , 2016 .

[7]  Shoji Kawahito,et al.  Kyoto's event-driven x-ray astronomy SOI pixel sensor for the FORCE mission , 2018, Astronomical Telescopes + Instrumentation.

[8]  Motohide Kokubun,et al.  Hard x-ray imager onboard Hitomi (ASTRO-H) , 2018 .

[9]  A. Takeda,et al.  Design and Evaluation of an SOI Pixel Sensor for Trigger-Driven X-Ray Readout , 2013, IEEE Transactions on Nuclear Science.

[10]  Manabu Ishida,et al.  The FORCE mission: science aim and instrument parameter for broadband x-ray imaging spectroscopy with good angular resolution , 2018, Astronomical Telescopes + Instrumentation.

[11]  Y. Arai,et al.  X-ray response evaluation in subpixel level for X-ray SOI pixel detectors , 2018, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment.

[12]  Y. Arai,et al.  Subpixel response of SOI pixel sensor for X-ray astronomy with pinned depleted diode: first result from mesh experiment , 2019, Journal of Instrumentation.

[13]  William W. Zhang,et al.  Next generation x-ray optics for astronomy: high resolution, lightweight, and low cost , 2019 .

[14]  Y. Arai,et al.  X-ray Performance of Back-Side Illuminated Type of Kyoto's X-ray Astronomical SOI Pixel Sensor, XRPIX , 2016, 1604.00170.

[15]  Shoji Kawahito,et al.  A Low-Noise X-ray Astronomical Silicon-On-Insulator Pixel Detector Using a Pinned Depleted Diode Structure , 2017, Sensors.