首页> 外文会议>Conference on UV, Optical, and IR Space Telescopes and Instruments 29-31 March 2000 Munich, Germany >A Near IR Fabry-Perot Interferometer for Wide Field,Low Resolution Hyperspectral Imaging on the Next generation Space Telescope
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A Near IR Fabry-Perot Interferometer for Wide Field,Low Resolution Hyperspectral Imaging on the Next generation Space Telescope

机译:用于下一代太空望远镜的宽视野,低分辨率高光谱成像的近红外法布里-珀罗干涉仪

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We discuss work in progress on a near-infrared tunable bandpass filter for the Goddard baseline wide field camera concept of the Next Generation Space Telescope (NGST) Integrated Science Instrument Module (ISIM). This filter, the Demonstration Unit for Low Order Cryogenic Etalon (DULCE), is designed to demonstrate a high efficiency scanning Fabry-Perot etalon operating in interference orders 1 - 4 at 30K with a high stability DSP based servo control system. DULCE is currently the only available tunable filter for lower order cryogenic operation int he near infrared. In this application, scanning etalons will illuminate the focal plane arrays with a single order of interference to enable wide field lower resolution hyperspectral imaging over a wide range of redshifts. We discuss why tunable filters are an important instrument component in future space-based observatories.
机译:我们讨论了下一代太空望远镜(NGST)集成科学仪器模块(ISIM)的Goddard基线宽视场摄像机概念的近红外可调谐带通滤波器的开发工作。该滤波器是低阶低温标准具的演示单元(DULCE),旨在演示采用基于DSP的高稳定性伺服控制系统,以1-3的干扰量工作在3-4干扰等级下的高效扫描Fabry-Perot标准具。 DULCE是目前唯一可用于近红外低阶低温操作的可调滤波器。在此应用中,扫描标准具将以单级干扰照亮焦平面阵列,从而能够在宽范围的红移范围内进行广域低分辨率高光谱成像。我们讨论了为什么可调滤波器在未来的天基观测站中是重要的仪器组成部分。

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