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Developing Wide-Field Spatio-Spectral Interferometry for Far-Infrared Space Applications

机译:开发用于远红外空间应用的广域时空光谱干涉仪

摘要

Interferometry is an affordable way to bring the benefits of high resolution to space far-IR astrophysics. We summarize an ongoing effort to develop and learn the practical limitations of an interferometric technique that will enable the acquisition of high-resolution far-IR integral field spectroscopic data with a single instrument in a future space-based interferometer. This technique was central to the Space Infrared Interferometric Telescope (SPIRIT) and Submillimeter Probe of the Evolution of Cosmic Structure (SPECS) space mission design concepts, and it will first be used on the Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII). Our experimental approach combines data from a laboratory optical interferometer (the Wide-field Imaging Interferometry Testbed, WIIT), computational optical system modeling, and spatio-spectral synthesis algorithm development. We summarize recent experimental results and future plans.
机译:干涉测量法是将高分辨率的好处带入太空远红外天体物理学的一种经济实惠的方法。我们总结了正在进行的努力,以开发和学习干涉测量技术的实际局限性,该技术将使未来的天基干涉仪能够使用单个仪器来采集高分辨率远红外积分场光谱数据。这项技术是空间红外干涉望远镜(SPIRIT)和宇宙结构演变的亚毫米探针(SPECS)太空任务设计概念的核心,它将首先在用于红外干涉的气球实验双筒望远镜(BETTII)中使用。我们的实验方法结合了实验室光学干涉仪(宽场成像干涉仪测试台,WIIT),计算光学系统建模和时空光谱综合算法开发的数据。我们总结了最近的实验结果和未来的计划。

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