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DUET:用于超冷矮星系外行星凌星观测的同时InGaAs-CCD分束成像仪设计

DUET: Design of a simultaneous InGaAs--CCD split-beam imager for ultra-cool dwarf exoplanet transit survey

Peter P. Pedersen, Clark Baker, Karolina Dziewiecka, Mathias Beck, Michaël Gillon, Amaury H. M. J. Triaud, Didier Queloz

arXiv 2607.14772首次发表:更新:

AI 中文总结

为探测超冷矮星系外行星,设计DUET双通道成像仪,用955纳米二向色分束器将光分至不同探测器实现同时测光,选近红外滤光片抑制PWV影响,还介绍了光学、机械、探测器及控制系统等设计。

AI 中文摘要

我们展示了DUET的设计,它是为SPECULOOS南方天文台(SSO)建造的双通道成像仪,用于探测和表征围绕超冷矮星运行的凌日类地系外行星。一个955纳米的二向色分束器将可见光导向深度耗尽的硅CCD,近红外光导向基于CMOS的InGaAs探测器,实现0.4至1.7微米波段的完全同时测光。选择近红外滤光片以抑制对大气可降水汽(PWV)变化的敏感度,这是冷恒星地基红外测光中相关噪声的主要来源。我们描述了光学和机械结构、二向色镜和滤光片选择、探测器选择以及控制系统。

英文摘要

We present the design of DUET, a dual-channel imager being built for the SPECULOOS-Southern Observatory (SSO) to detect and characterise transiting terrestrial exoplanets orbiting ultra-cool dwarfs. A dichroic beamsplitter at 955\,nm directs visible light to a deeply-depleted silicon CCD and near-infrared light to a CMOS-based InGaAs detector, enabling fully simultaneous photometry with bandpasses from 0.4 to 1.7\,\textmu m. The near-infrared filters have been chosen to suppress sensitivity to atmospheric precipitable water vapour (PWV) variability, a dominant source of correlated noise in ground-based infrared photometry of cool stars. We describe the optical and mechanical architecture, the dichroic and filter selection, the choice of detectors, and the control system.

Comments12 pages, 8 figures, 2 Tables, proceedings of SPIE Astronomical Telescopes + Instrumentation 2026, 14149-438

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