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French SWIR technology used for astronomy

机译:法国用于天文学的SWIR技术

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During the last 30 years, the Space Research Department (DESPA) of Paris Observatory has developed infrared instrumentation for space and ground-based telescopes. First, we present the PbS linear detector of the ISM IR imaging spectrometer of the Phobos mission. Then the CID InSb focal plane of ISOCAM-SW is described. The studies of this CID InSb focal plane allowed us to develop an IR camera for the first astronomical observations using adaptive optics. We also describe the linear array built for the OMEGA imaging spectrometer of the Mars 96 mission. The last chapter is dedicated to the IR spectrometer of the Huygens probe. To conclude, the needs and challenges in the area of mid-band infrared astronomy are discussed.
机译:在过去的30年中,巴黎天文台的太空研究部(DESPA)开发了用于太空和地面望远镜的红外仪器。首先,我们介绍了Phobos任务的ISM红外光谱仪的PbS线性探测器。然后描述了ISOCAM-SW的CID InSb焦平面。对这种CID InSb焦平面的研究使我们能够开发出红外相机,以使用自适应光学器件进行首次天文观测。我们还描述了为火星96任务的OMEGA成像光谱仪构建的线性阵列。上一章专门介绍惠更斯探头的红外光谱仪。总之,讨论了中频红外天文学领域的需求和挑战。

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