Infrared detectors for ground-based and space-based astronomy applications
Infrared detectors for ground-based and space-based astronomy applications
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用于地基和空基天文学应用的红外探测器
DOI：
10.1117/12.395462
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发表时间：
2000
期刊：
影响因子：
--
通讯作者：
K. Sparkman
中科院分区：
文献类型：
--
作者：
P. Love;K. J. Ando;J. Garnett;N. Lum;J. Rosbeck;Michael S. Smith;K. Sparkman
本文将回顾雷神红外卓越中心的最先进的红外探测器，用于地面和天基天文学应用。性能数据将在0.5至5.0微米的锑化铟（InSb）阵列和0.9至5.0微米的碲镉汞阵列。此外，2至28微米的掺砷硅杂质带导体阵列的性能数据将提交。这些高性能探测器阵列为地面和空间天文工作提供了另一个重要的宇宙窗口。数据将包括用于美国航天局空间红外望远镜设施的红外阵列照相机仪器和ISAS ASTRO-F红外成像巡天（IRIS）使命任务的红外成像仪的InSb和Si：As IBC阵列的性能数据。还将介绍为欧空局ROSETTA使命的可见光和红外热成像光谱仪H和M仪器开发的碲镉汞阵列获得的数据。将重点介绍地基和天基天文学应用的读数，包括下一代空间望远镜的第一个原型多路复用器和4 K X 4 K焦平面阵列。
This paper will review the state-of-the-art IR detectors at the Raytheon IR Center of Excellence for both grou8nd-based and space-based astronomy applications. Performance data will be presented on 0.5 to 5.0 micron Indium Antimonide (InSb) arrays and 0.9 to 5.0 micron Mercury Cadmium Telluride arrays. In addition, performance data on 2 to 28 micron Arsenic-doped Silicon impurity band conductor arrays will be presented. These very high performance detector array offer another important window into the universe for ground- and space-based astronomical work. Data will include performance data on InSb and Si:As IBC arrays for the IR array camera instrument on NASA's Space IR Telescope Facility and the IRC instrument on the ISAS ASTRO-F IR Imaging Survey (IRIS) mission. Data obtained with the HgCdTe arrays developed for the Visible and IR Thermal Imaging Spectrometer H and M instruments for the ESA ROSETTA mission will also be presented. Readouts for both ground-based and space-based astronomy applications will be highlighted, including the first prototype multiplexer and 4 K X 4 K Focal Plane Array for the next generation space telescope.