High-resolution fibre-fed spectrograph for the 6-m telescope. Polarimetric unit


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Abstract

We report the computation of the design of a polarimetric unit for the optical scheme of the fiberfed high-resolution spectrograph for the 6-m Russian telescope.We discuss a variant of its integration into the design of conversion optics at the input of the fiber path if the instrument and estimate the efficiency of the entire pre-fiber optical system. The luminous efficiency of the assembly is equal to 80 and 90% when operated in the polarimetry and normal spectroscopic modes, respectively.We estimate the lower limit for the distorting instrumental effects of the polarimetric unit.

About the authors

D. E. Kukushkin

St. Petersburg National Research University of Information Technologies, Mechanics and Optics

Author for correspondence.
Email: intenso.dk@gmail.com
Russian Federation, St. Petersburg, 197101

D. A. Sazonenko

St. Petersburg National Research University of Information Technologies, Mechanics and Optics

Email: intenso.dk@gmail.com
Russian Federation, St. Petersburg, 197101

A. V. Bakholdin

St. Petersburg National Research University of Information Technologies, Mechanics and Optics

Email: intenso.dk@gmail.com
Russian Federation, St. Petersburg, 197101

M. V. Yushkin

Special Astrophysical Observatory

Email: intenso.dk@gmail.com
Russian Federation, Nizhnii Arkhyz, 369167

V. D. Bychkov

Special Astrophysical Observatory

Email: intenso.dk@gmail.com
Russian Federation, Nizhnii Arkhyz, 369167

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