Atlas of Vega: 3850 -- 6860 \AA
Hyun-Sook Kim, Inwoo Han, G. Valyavin, Byeong-Cheol Lee, V. Shimansky,, G.A. Galazutdinov

TL;DR
This paper provides a high-resolution, high signal-to-noise spectral atlas of Vega spanning 3850 to 6860 Å, useful for stellar analysis and calibration.
Contribution
It presents a detailed spectral atlas of Vega with unprecedented resolution and quality, compiled from multiple high-quality observations.
Findings
High resolving power of 90,000 achieved.
Signal-to-noise ratio around 700.
Spectral data made available electronically.
Abstract
We present a high resolving power ( / = 90,000) and high signal-to-noise ratio (700) spectral atlas of Vega covering the 3850 -- 6860 \AA wavelength range. The atlas is a result of averaging of spectra recorded with the aid of the echelle spectrograph BOES fed by the 1.8-m telescope at Bohyunsan observatory (Korea). The atlas is provided only in machine-readable form (electronic data file) and will be available in the SIMBAD database upon publication.
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