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Detectors and cryostat design for the SuMIRe Prime Focus Spectrograph (PFS)

机译:SuMIRe Prime Focus Spectrograph(PFS)的检测器和低温恒温器设计

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We describe the conceptual design of the camera cryostats, detectors, and detector readout electronics for the SuMIRePrime Focus Spectrograph (PFS) being developed for the Subaru telescope. The SuMIRe PFS will consist of fouridentical spectrographs, each receiving 600 fibers from a 2400 fiber robotic positioner at the prime focus. Eachspectrograph will have three channels covering wavelength ranges 3800 Å - 6700 Å, 6500 Å - 10000 Å, and 9700 Å -13000 Å, with the dispersed light being imaged in each channel by a f/1.10 vacuum Schmidt camera. In the blue and redchannels a pair of Hamamatsu 2K x 4K edge-buttable CCDs with 15 um pixels are used to form a 4K x 4K array. Forthe IR channel, the new Teledyne 4K x 4K, 15 um pixel, mercury-cadmium-telluride sensor with substrate removed forshort-wavelength response and a 1.7 um cutoff will be used. Identical detector geometry and a nearly identical opticaldesign allow for a common cryostat design with the only notable difference being the need for a cold radiation shield inthe IR camera to mitigate thermal background. This paper describes the details of the cryostat design and coolingscheme, relevant thermal considerations and analysis, and discusses the detectors and detector readout electronics.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:我们描述了为斯巴鲁望远镜开发的SuMIRePrime聚焦光谱仪(PFS)的相机低温恒温器,探测器和探测器读出电子设备的概念设计。 SuMIRe PFS将由四个相同的光谱仪组成,每个光谱仪主要从2400光纤自动定位器接收600根光纤。每个光谱仪将具有三个通道,分别覆盖波长范围3800Å-6700Å,6500Å-10000Å和9700 -13000Å​​,分散的光通过f / 1.10真空Schmidt相机在每个通道中成像。在蓝色和红色通道中,使用一对具有15 um像素的Hamamatsu 2K x 4K边缘对接CCD来形成4K x 4K阵列。对于IR通道,将使用新型Teledyne 4K x 4K,15 um像素,汞-碲化镉汞传感器,并去除了基板以实现短波长响应和1.7 um截止。相同的探测器几何形状和几乎相同的光学设计可实现通用的低温恒温器设计,唯一的显着差异是IR摄像机中需要冷辐射屏蔽以减轻热本底。本文介绍了低温恒温器设计和冷却方案的详细信息,相关的热量考虑因素和分析,并讨论了探测器和探测器读数电子设备。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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