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A spectropolarimetric focal station for the ESO E-ELT

机译:ESO E-ELT的光谱偏振聚焦站

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We present a conceptual design for a spectropolarimetric focal station for ESO's European Extremely Large Telescope(E-ELT). It uses the intermediate f/4.4 focus, the only symmetric focus of the telescope. A dual channel, full Stokesvectorpolarimeter provides on-axis light for the wavelength range 380-1600nm to up to two spectrographssimultaneously via two pairs of fibers. With such spectropolarimetric capability and a proper spectrograph for the opticaland the near infrared wavelengths, the E-ELT would be able to provide the full parameter space of an incomingwavefront. Because of the on-axis entrance location of the polarimeter collimator and an entrance aperture of just 1.3arcsec, the expected poor image quality of the intermediate telescope focus is not directly relevant.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:我们为ESO的欧洲超大型望远镜(E-ELT)的光谱极化聚焦站提出了一种概念设计。它使用中间的f / 4.4焦点,这是望远镜的唯一对称焦点。双通道全Stokesvector旋光仪可通过两对光纤同时提供380-1600nm波长范围内的同轴光,最多可同时提供两个光谱仪。有了这样的光谱极化能力并为光学和近红外波长配备合适的光谱仪,E-ELT将能够提供入射波前的完整参数空间。由于旋光仪准直器在轴上的入射位置以及入射光孔径仅为1.3arcsec,因此中间望远镜聚焦的预期不良图像质量不是直接相关的。©(2012)COPYRIGHT光电仪器工程师协会(SPIE) )。摘要的下载仅允许个人使用。

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