Paper
17 September 2012 A spectropolarimetric focal station for the ESO E-ELT
Klaus G. Strassmeier, Igor DiVarano, Ilya Ilyin, Manfred Woche, Uwe Laux
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Abstract
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 Stokesvector polarimeter provides on-axis light for the wavelength range 380-1600nm to up to two spectrographs simultaneously via two pairs of fibers. With such spectropolarimetric capability and a proper spectrograph for the optical and the near infrared wavelengths, the E-ELT would be able to provide the full parameter space of an incoming wavefront. Because of the on-axis entrance location of the polarimeter collimator and an entrance aperture of just 1.3 arcsec, 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.
Klaus G. Strassmeier, Igor DiVarano, Ilya Ilyin, Manfred Woche, and Uwe Laux "A spectropolarimetric focal station for the ESO E-ELT", Proc. SPIE 8444, Ground-based and Airborne Telescopes IV, 844435 (17 September 2012); https://doi.org/10.1117/12.926009
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KEYWORDS
Polarimetry

Telescopes

Optical fibers

Mirrors

Space telescopes

Collimators

Adaptive optics

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