Fig. 15

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Normalized χ2/NDOF of VELOCE Fourier series fits vs. the median uncertainty of the RV measurements for 151 non-SB1 Cepheids. The rapid increase of χ2/NDOF for precise measurements with typical uncertainties better than 20–40 m s−1 shows the existence of additional signals that are not reproduced by Fourier series models with constant Ppuls. The three longest-period Cepheids in the sample, GS Lup, SV Vul, and S Vul are labeled and highlighted.
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