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Fig. 1
Histogram of std(RV) per star of the 287 stars that were observed at least five times before September 2017. The RVs used for this plot were derived from the CARMENES VIS spectra with SERVAL (Zechmeister et al. 2018). The dashed line is the adopted boundary between RV-quiet and RV-loud stars at std(RV) = 10 m s−1.
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