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The first diluted telescope ever built in the world

机译:曾经在世界上建造的第一个摊薄望远镜

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We have built at the Haute-Provence observatory (France) the rst diluted telescope in the world. We describethis prototype called Carlina, made of three 25 cm mirrors separated by a maximum baseline of 10.5 m. Thethree mirrors in place are already coherenced and rst light is scheduled for June-July 2012. In this article, wewill mainly describe the focal gondola. We propose to build in the near future a 100 m aperture Large DilutedTelescope. This diluted telescope will be more sensitive than regular interferometers (Keck, VLTI, etc.), withhigher imaging capabilities. A LDT will open new elds of research in astrophysics thanks to very high angularresolution imaging of the surface of supergiant stars, AGN, gravitational micro-lens systems, exo-planets, etc.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:我们建立在普瑞斯普罗旺斯天文台(法国)世界上第一座稀释的望远镜。我们描述了称为Carlina的原型,由三个25厘米的镜子分开,最大基线为10.5米。 TheThree镜子到位已经结束,RST灯计划于2012年6月至7月。在本文中,威尔主要描述了焦点贡多拉。我们建议在不久的将来建立100米孔径大量稀释的薄膜。这种稀释的望远镜比常规干涉仪(Keck,VLTI等)更敏感,具有高度的成像能力。 LDT将在Superigiant Stars,Agn,引力微透镜系统,外部行星级别的表面的非常高的Angular Resolution成像非常高的Angular Resolution成像。©(2012)版权协会的光学仪表工程师( spie)。仅供个人使用的摘要下载。

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