Fig. 6
Residuals of the effective temperatures obtained through the Teff vs. V−Ks calibrations of Ramírez & Meléndez (2005) (top panel, red), González Hernández & Bonifacio (2009) (middle panel, green), and Huang et al. (2015) (bottom panel, purple). These residuals are shown with respect to the values derived with the 
vs. G−Ks fit of this work for a sample of 179 APOGEE stars with high photometric quality and low interstellar extinction.
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