Echelle spectrograph at the 2.6 m Shajn telescope

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Published: Apr 15, 2020
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DOI: https://doi.org/10.31059/aat.vol1.iss1.pp33-38
Keywords:
astronomy instruments observational facilities spectrometry

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Aleksandr Lagutin
Crimean Astrophysical Observatory, Nauchny 298409, Crimea
Sergei Plachinda
Crimean Astrophysical Observatory, Nauchny 298409, Crimea
Dmitrii Shakhovskoi
Crimean Astrophysical Observatory, Nauchny 298409, Crimea
Evgenii Nekhai
Crimean Astrophysical Observatory, Nauchny 298409, Crimea
Dilyara Baklanova
Crimean Astrophysical Observatory, Nauchny 298409, Crimea
Petr Petrov
Crimean Astrophysical Observatory, Nauchny 298409, Crimea

Abstract

The paper describes the high-resolution echelle spectrograph ESPL developed for the coude focus of the 2.6 m Shajn reflector of the Crimean Astrophysical Observatory.  The spectrograph has been regularly operated since 2013.  Efficiency of the spectrograph is estimated from observations of stars.

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How to Cite
Lagutin A., Plachinda S., Shakhovskoi D. , et al., 2020. Acta Astrophysica Taurica, vol. 1, no. 1, pp. 33–38. DOI: 10.31059/aat.vol1.iss1.pp33-38
Issue
Vol. 1 No. 1 (2020)
Section
Research articles
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