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Table B.1

Spectral regions analyzed with ROTFIT.

Range Main features T eff log g r vsini RV

9590–9800 Ti i, Cr i Ya N Y Y Y
8160–8222 Na i Y Y Y N Y
7600–7720 K i Y Y Y N Y
7020–7120 TiO Y N Y N Y
6050–6270 Ca i, Fe i, TiO Y Y Y Yb Y
5320–5500 Fe i Yb Yb Yb N N
5120–5220 Mg i b Yb Yb Yb N N
4400–4580 Fe i Yb Yb Yb N N

Notes.

(a)

Low sensitivity to this parameter.

(b)

For the best exposed spectra of stars hotter than about 3500 K.

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