ADAM low- and medium-resolution spectrograph for 1.6-m AZT-33IK telescope


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Abstract

We describe the design of a suspended low- and medium-resolution spectrograph (R ≈ 300–1300) designed and made at the Special Astrophysical Observatory of the Russian Academy of Sciences for the 1.6-m AZT-33IK telescope of Sayan Observatory of the Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences. We report the results of laboratory measurements of the parameters of the instrument and tests performed on the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. We measured the total quantum efficiency of the “spectrograph + telescope + detector” system on AZT-33IK telescope, which at its maximum reaches 56%. Such a hight transparency of the spectrograph allows it to be used with the 1.6-m telescope to determine the types and redshifts of objects with integrated magnitudes mAB ≈ 20–21, and this result was confirmed by actual observations.

About the authors

V. L. Afanasiev

Special Astrophysical Observatory

Author for correspondence.
Email: vafan@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167

S. N. Dodonov

Special Astrophysical Observatory

Email: moisav@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167

V. R. Amirkhanyan

Special Astrophysical Observatory; Sternberg Astronomical Institute

Email: moisav@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167; Moscow, 119992

A. V. Moiseev

Special Astrophysical Observatory

Author for correspondence.
Email: moisav@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167


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