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Fig. 1


Noise-free simulated RVS spectra for late B- to K-spectral-type metal-rich dwarf stars, included in the reference grids. The adopted effective temperatures are 11 000 K, 9000 K, 7500 K, 6500 K, 5500 K, and 4500 K from bottom to top, respectively. The other stellar parameters are kept constant at log(g) = 4.5 cm/s2, [M/H] = +0.0 dex, and [α/Fe] = +0.0 dex. The identified lines refer to most of the strongest atomic transitions that are present in the different spectra.

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