Fig. A.1
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Three examples illustrating the reasons why some RAVE spectra were rejected: a) A spectrum of the F6 dwarf (Houk & Cowley 1975) HD 2493 illustrating a case of low S/N. b) A spectrum of the A9 dwarf (Houk & Smith-Moore 1988) HD 106609 illustrating contamination by Paschen lines. c) A spectrum of the F2 dwarf (Houk & Smith-Moore 1988) HD 104910 illustrating a case of odd feature seen in the spectrum. Ca II IRT lines are marked with red vertical lines.
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