We designed a cross-dispersion fiber-fed spectrograph for moderate-diameter telescopes. The instrument can simultaneously record the wavelength interval spanning from 3850 to 10 850 ˚A at a spectral resolution of R = 45 000 with the maximum diameter of the input star image of 3 .3. The instrument allows the spectrum of the star to be recorded simultaneously with the comparison spectrum. Spectra can also be acquired with the use of linear and circular polarization analyzers. The instrument is oriented toward high-precision monitoring of line properties in stellar spectra.
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