Demonstrating repetitive non-destructive readout with SiSeRO devices

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-01-01 DOI:10.1117/1.jatis.10.1.016004
Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, Kevan Donlon, Gregory Prigozhin, Glenn Morris, Michael Cooper, Beverly LaMarr, Andrew Malonis, Steven W. Allen, Marshall W. Bautz, Chris Leitz
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Abstract

We demonstrate so-called repetitive non-destructive readout (RNDR) for the first time on a single electron sensitive readout (SiSeRO) device. SiSeRO is a novel on-chip charge detector output stage for charge-coupled device image sensors, developed at MIT Lincoln Laboratory. This technology uses a p-MOSFET transistor with a depleted internal gate beneath the transistor channel. The transistor source-drain current is modulated by the transfer of charge into the internal gate. RNDR was realized by transferring the signal charge non-destructively between the internal gate and the summing well (SW), which is the last serial register. The advantage of the non-destructive charge transfer is that the signal charge for each pixel can be measured at the end of each transfer cycle, and by averaging for a large number of measurements (Ncycle), the total noise can be reduced by a factor of 1/Ncycle. In our experiments with a prototype SiSeRO device, we implemented nine (Ncycle=9) RNDR cycles, achieving around two electron readout noise (equivalent noise charge or ENC) with a spectral resolution close to the fano limit for silicon at 5.9 keV. These first results are extremely encouraging, demonstrating successful implementation of the RNDR technique in SiSeROs. They also lay the foundation for future experiments with more optimized test stands (better temperature control, larger number of RNDR cycles, and RNDR-optimized SiSeRO devices), which should be capable of achieving sub-electron noise sensitivities. This new device class presents an exciting technology for next generation astronomical X-ray telescopes requiring very low-noise spectroscopic imagers. The sub-electron sensitivity also adds the capability to conduct in-situ absolute calibration, enabling unprecedented characterization of the low energy instrument response.
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利用 SiSeRO 设备演示重复性无损读数
我们首次在单电子敏感读出(SiSeRO)器件上演示了所谓的重复无损读出(RNDR)。SiSeRO 是麻省理工学院林肯实验室为电荷耦合器件图像传感器开发的一种新型片上电荷检测器输出级。该技术采用 p-MOSFET 晶体管,晶体管沟道下方有一个耗尽型内部栅极。晶体管的源极-漏极电流通过向内部栅极转移电荷来调节。RNDR 是通过在内部栅极和作为最后一个串行寄存器的求和井 (SW) 之间非破坏性地传输信号电荷来实现的。无损电荷转移的优势在于,每个像素的信号电荷可在每个传输周期结束时测量,通过对大量测量(N 个周期)进行平均,总噪声可降低 1/N 个周期。在使用 SiSeRO 原型设备的实验中,我们实现了九次(Ncycle=9)RNDR 循环,读出噪声(等效噪声电荷或 ENC)约为两个电子,光谱分辨率接近 5.9 keV 时硅的扇形极限。这些初步结果非常令人鼓舞,证明了 RNDR 技术在 SiSeRO 中的成功应用。它们还为未来使用更优化的测试台(更好的温度控制、更多的 RNDR 周期和 RNDR 优化的 SiSeRO 器件)进行实验奠定了基础,这些实验应该能够实现亚电子噪声灵敏度。这种新型器件为需要极低噪声光谱成像仪的下一代天文 X 射线望远镜提供了令人兴奋的技术。亚电子灵敏度还增加了进行原位绝对校准的能力,从而能够对低能仪器的响应进行前所未有的鉴定。
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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