Fig. C.1.

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Example of spectral fits for the cool, slow rotator GES 10353450–5813461 with Teff = 11 760 K and V sin i = 42 km s−1 (top left panel), the cool, fast rotator GES 10353820–5811092 with Teff = 10 800 K and V sin i = 276 km s−1 (top right panel), the hot, slow rotator GES 10355660–5811314 with Teff = 22 701 K and V sin i = 27 km s−1 (bottom left panel), and the hot, fast rotator GES 10360349–5814401 with Teff = 20 322 K and V sin i = 257 km s−1 (bottom right panel). The observations are shown in black and the fits in red. Two stars do not have HR04 data available.
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