High-resolution fibre-fed spectrograph for the 6-m telescope. Polarimetric unit
- Authors: Kukushkin D.E.1, Sazonenko D.A.1, Bakholdin A.V.1, Yushkin M.V.2, Bychkov V.D.2
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Affiliations:
- St. Petersburg National Research University of Information Technologies, Mechanics and Optics
- Special Astrophysical Observatory
- Issue: Vol 71, No 2 (2016)
- Pages: 249-256
- Section: Article
- URL: https://journal-vniispk.ru/1990-3413/article/view/212217
- DOI: https://doi.org/10.1134/S1990341316020127
- ID: 212217
Cite item
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.
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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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