Fig. 10.
Histograms of the rms distance (Eq. (4)) separately for stars classified as CEMP-s, CEMP-rs or r-star in Col. 8 of Table 1. Since the re-assignment procedure is based on a threshold value using the signed distance (dS = 0.6, Eq. (3) and Fig. 9), we cannot plot a similar threshold in the present drms histogram.
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