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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment >Performance verification of next-generation Si CMOS soft X-ray detector for space applications
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Performance verification of next-generation Si CMOS soft X-ray detector for space applications

机译:用于空间应用的下一代Si CMOS软X射线检测器的性能验证

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All-sky surveys of X-ray transient objects in the soft X-ray band are essential for observing high-redshift events to probe unexplored physical conditions in the early universe and discovering mysterious electromagnetic counterparts of gravitational-wave sources. HiZ-GUNDAM is a future satellite mission that intends to perform a wide-field survey in the soft X-ray band (0.4-4 kcV). The HiZ-GUNDAM X-ray detector has Si pixel sensors that require fine positioning accuracy (e.g. tens of micrometers), high detection efficiency, a large detection area (tens of cm~2) and, a relatively high frame rate of ~10 frames per second that can be achieved by a back-illuminated Si CMOS image sensor. One of the most promising candidates is GSENSE6060BSI with 6144 x 6144 pixels fabricated by Gpixel Inc. In this paper, for the initial performance test, we used a smaller-sized CMOS sensor, GSENSE400BSI-TVISB, which is similar to GSENSE6060BSI in terms of pixel characteristics, such as pixel size, epilayer thickness, and resistivity, except for the number of pixels (2048 × 2048). We conducted a detailed study on the spectroscopic performance of GSENSE400BSI-TVISB in the soft X-ray band and its radiation tolerance for space applications. For the spectroscopic performance, low-energy X-ray lines such as Al-K_α (1.5 kcV), Mn-K_α (5.9 keV), and Mn-K_β, (6.5 keV) were clearly detected. Furthermore, using the obtained X-ray events, we estimated >50% detection efficiency in the 0.4-4 keV band, corresponding to a ~10-μm Si thickness of the detectable layer. We also performed radiation tolerance tests against gamma rays from ~60Go, 100-MeV protons and 5.5-MeV alpha rays (5-30 krad, corresponding to 6-30 year operation in orbit). After the irradiation tests, we observed that GSENSE400BSI-TVISB has strong radiation tolerance for our purpose: the lower detectable energy of ~0.4 keV can be obtained if the CMOS is operated with an exposure of 0.1 s at -20 °C.
机译:软X射线频段中的X射线瞬态物体的全天调查对于观察高射频事件,对于早期宇宙中未开发的物理条件探讨并发现引力波来源的神秘电磁对应物,这是必不可少的。 Hiz-Gundam是一个未来的卫星使命,打算在软X射线带(0.4-4 kcv)中进行广泛的田间调查。 Hiz-Gundam X射线检测器具有SI像素传感器,需要精细定位精度(例如,数微米),高检测效率,大检测区域(几十厘米〜2),并且相对高的帧速率为约10帧每秒可以通过后照射Si CMOS图像传感器实现。最有前途的候选人之一是GSENSE6060BSI,由GPixel Inc.制造的6144 x 6144像素。在本文中,对于初始性能测试,我们使用了一个较小的CMOS传感器,GSENSE400BSI-TVISB,它与像素相似的GSENSE6060BSI除了像素的数量之外,例如像素尺寸,脱毛厚度和电阻率之类的特性(2048×2048)。我们对软X射线带中GSENSE400BSI-TVISB的光谱性能进行了详细研究及其空间应用的辐射公差。对于光谱性能,清楚地检测到诸如Al-Kα(1.5kCV),Mn-Kα(5.9kC)和Mn-K_β,(6.5keV)的低能量X射线线。此外,使用所获得的X射线事件,我们估计了0.4-4KeV带中的50%检测效率,对应于可检测层的〜10μmSi厚度。我们还对来自〜60Go,100meV质子和5.5meVα射线(5-30 krad的5-30 krad进行了5-30 krad的γ射线进行了针对γ射线的辐射耐受性测试。在照射测试之后,我们观察到GSENSE400BSI-TVISB为我们目的具有强大的辐射耐受性:如果在-20℃下的曝光为0.1秒,则可以获得〜0.4keV的较低可检测能量。

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