Low-energy X-ray performance of SOI pixel sensors for astronomy, “XRPIX”
Low-energy X-ray performance of SOI pixel sensors for astronomy, “XRPIX”
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天文学用 SOI 像素传感器“XRPIX”的低能 X 射线性能
DOI:
10.1016/j.nima.2020.164745
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发表时间:
2021
期刊:
影响因子:
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通讯作者:
et al.
中科院分区:
文献类型:
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作者:
Kodama Ryota;Ayaki Takeda;et al.
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 FK 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 FK 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.