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Technology challenges for space interferometry: The option of mid-infrared integrated optics
Authors:L Labadie  P Kern  P Labeye  E LeCoarer  C Vigreux-Bercovici  A Pradel  J-E Broquin  V Kirschner
Institution:1. Max-Planck Institut für Astronomie, Königstuhl, 17, D-69117 Heidelberg, Germany;2. Laboratoire d’Astrophysique de Grenoble, BP53, F-38041 Grenoble Cedex 9, France;3. Laboratoire d’Electronique et des Technologies de l’Information (CEA), 17, rue des Martyrs, 38054 Grenoble Cedex 9, France;4. Laboratoire de Physico-Chimie de la Matière Condensée, Institut Gehrardt, Place Eugène Bataillon, 34095 Montpellier Cedex 5, France;5. Institut de Microelectronique et Electromagnétisme et Photonique, 23, rue des Martyrs, 38016 Grenoble Cedex 1, France;6. ESTEC-ESA, P.O. Box 299, 2200 AG Noordwijk, The Netherlands
Abstract:Nulling interferometry is a technique providing high angular resolution which is the core of the space missions Darwin and TPF. The first objective is to reach a deep degree of starlight cancelation in the range 6–20 μm, in order to observe and to characterize the signal from an earth-like planet. Among the numerous technological challenges involved in these missions, the question of the beam combination and wavefront filtering has an important place. A single-mode integrated optics (IO) beam combiner could support both the functions of filtering and the interferometric combination, simplifying the instrumental design. Such a perspective has been explored in this work within the project Integrated Optics for Darwin (IODA), which aims at developing a first IO combiner in the mid-infrared. The solutions reviewed here to manufacture the combiner here are based on infrared dielectric materials on one side, and on metallic conductive waveguides on the other side. With this work, additional inputs are offered to pursue the investigation on mid-infrared photonics devices.
Keywords:Space-based nulling interferometry  Single-mode integrated optics  Mid-infrared instrumentation
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