Paper
6 July 2018 Wide-field acousto-optical imaging spectral polarimeter: design and commissioning
Sergey P. Anikin, Alexander I. Chizhikov, Valentin F. Esipov, Vasily V. Gurov, Alexander I. Kolesnikov, Vladimir Y. Molchanov, Sergey A. Potanin, Andrey M. Tatarnikov, Konstantin B. Yushkov
Author Affiliations +
Abstract
We report design of acousto-optic imaging spectrometer for spectral and polarimetric photometry and commis- sioning of the instrument at 0.6-m F/12.5 telescope at the Southern Astronomical Station of Lomonosov Moscow State University. The spectrometer was operating over the spectral range 3800–5800 Å with the passband of 10 Å at the wavelength of 5000 Å The imaging spectrometer could be used for observations of objects with the minimum brightness of 12.5 mag (for 0.6-m telescope, 120 s exposition, and SNR∼10). Spatial resolution of the spectrometer was estimated better than 1.2”, and the field of view was ∼250”.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sergey P. Anikin, Alexander I. Chizhikov, Valentin F. Esipov, Vasily V. Gurov, Alexander I. Kolesnikov, Vladimir Y. Molchanov, Sergey A. Potanin, Andrey M. Tatarnikov, and Konstantin B. Yushkov "Wide-field acousto-optical imaging spectral polarimeter: design and commissioning", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 1070233 (6 July 2018); https://doi.org/10.1117/12.2313474
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KEYWORDS
Spectroscopy

Polarization

Diffraction

Polarimetry

Telescopes

Polarizers

Signal to noise ratio

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