用于 SOAR 积分场摄谱仪的 Skipper CCD 的特性分析与优化

IF 3.3 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Edgar Marrufo Villalpando, Alex Drlica-Wagner, Andrés A. Plazas Malagón, Abhishek Bakshi, Marco Bonati, Julia Campa, Braulio Cancino, Claudio R. Chavez, Juan Estrada, Guillermo Fernandez Moroni, Luciano Fraga, Manuel E. Gaido, Stephen Holland, Rachel Hur, Michelle Jonas, Peter Moore, Javier Tiffenberg
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引用次数: 0

摘要

我们介绍了用于南方天体物理研究所积分场摄谱仪(SIFS)焦平面原型的 Skipper 电荷耦合器件(CCD)的表征和优化结果。我们测试了八个 Skipper CCD,并根据性能结果为 SIFS 挑选了六个。Skipper CCD 是 6k × 1k、15 μm 像素、厚、全耗尽、p 沟道器件,经过减薄至 ∼ 250 μm、背面处理和抗反射涂层处理。我们证明,所有放大器的单样本读出噪声为 4.3 e- rms pixel-1。我们优化了读出序列时序,在 74 次非破坏性测量后,读出噪声达到了 0.5 e- rms 像素-1,在读出时间为 4 分钟的情况下,可以在检测器面积 5% 的区域内完成测量。我们在所有 24 个放大器(每个探测器有 4 个放大器)中演示了单光子计数,在 Nsamp = 400 个采样之后,读取噪声为 σN ∼ 0.18 e- rms pixel-1,并且在低信号水平(0 e- 至 50 e-)下,我们将非线性程度控制在 ≲1%。当斯基珀 CCD 配置为提供较大的全阱容量时,时钟诱导电荷(CIC)仍然是一个重要问题。在全阱容量为 ∼900 e- 时,我们的 CIC 率为 1.45 × 10-3 e- 像素-1 帧-1,在全阱容量为 ∼40,000-65,000 e- 时,CIC 率增至 ∼3 e- 像素-1 帧-1。我们还进行了常规 CCD 特性测量,如电荷转移低效率(平均 3.44 × 10-7)、暗电流(∼2 × 10-4 e- 像素-1 s-1)、光子转移曲线、外观缺陷(0.45% 的 "坏 "像素)和电荷扩散(点扩散函数 <7.5 μm),以验证这些特性与用于天文学的常规 p 沟道 CCD 的预期一致。此外,我们还首次利用 Skipper CCD 测量了更亮-更暗效应和绝对量子效率(450 至 980 纳米之间为 80%;600 至 900 纳米之间为 90%)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Characterization and Optimization of Skipper CCDs for the SOAR Integral Field Spectrograph
We present results from the characterization and optimization of Skipper charge-coupled devices (CCDs) for use in a focal plane prototype for the Southern Astrophysical Research Integral Field Spectrograph (SIFS). We tested eight Skipper CCDs and selected six for SIFS based on performance results. The Skipper CCDs are 6k × 1k, 15 μm pixels, thick, fully depleted, p-channel devices that have been thinned to ∼250 μm, backside processed, and treated with an anti-reflective coating. We demonstrate a single-sample readout noise of <4.3 e rms pixel−1 in all amplifiers. We optimize the readout sequence timing to achieve a readout noise of 0.5 e rms pixel−1 after 74 non-destructive measurements, which can be accomplished in a region covering 5% of the detector area in a readout time of <4 minutes. We demonstrate single-photon-counting in all 24 amplifiers (four amplifiers per detector) with a readnoise of σ N ∼ 0.18 e rms pixel−1 after N samp = 400 samples, and we constrain the degree of nonlinearity to be ≲1% at low signal levels (0 e to 50 e). Clock-induced charge (CIC) remains an important issue when the Skipper CCD is configured to provide a large full-well capacity. We achieve a CIC rate of <1.45 × 10−3 e pixel−1 frame−1 for a full-well capacity of ∼900 e, which increases to a CIC rate of ∼3 e pixel−1 frame−1 for full-well capacities ∼40,000–65,000 e. We also perform conventional CCD characterization measurements such as charge transfer inefficiency (3.44 × 10−7 on average), dark current (∼2 × 10−4 e pixel−1 s−1), photon transfer curves, cosmetic defects (<0.45% “bad” pixels), and charge diffusion (point-spread function < 7.5 μm) to verify that these properties are consistent with expectations from conventional p-channel CCDs used for astronomy. Furthermore, we provide the first measurements of the brighter-fatter effect and absolute quantum efficiency (≳80% between 450 and 980 nm; ≳90% between 600 and 900 nm) using Skipper CCDs.
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来源期刊
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific 地学天文-天文与天体物理
CiteScore
6.70
自引率
5.70%
发文量
103
审稿时长
4-8 weeks
期刊介绍: The Publications of the Astronomical Society of the Pacific (PASP), the technical journal of the Astronomical Society of the Pacific (ASP), has been published regularly since 1889, and is an integral part of the ASP''s mission to advance the science of astronomy and disseminate astronomical information. The journal provides an outlet for astronomical results of a scientific nature and serves to keep readers in touch with current astronomical research. It contains refereed research and instrumentation articles, invited and contributed reviews, tutorials, and dissertation summaries.
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