Fig. 4.

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Average of three spectra of St 2-22 obtained during quiescence in June and July 2017, compared with the spectra from the grid BT-NextGen of the theoretical spectra (Allard et al. 2011, log g = 0.5 dex and Teff in the range 3300−3600 K). The spectrum of St 2-22 most resembles the giant’s spectrum with Teff = 3400 K. The spectrum of the atmospheric transmission is shown at the bottom in magenta; it was not subtracted from the observed spectra. It was generated with the use of the TAPAS2 service (Bertaux et al. 2014), adopting conditions similar to those during our observations in Sutherland.
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