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Fig. 6


Residuals of the effective temperatures obtained through the Teff vs. VKs 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. GKs fit of this work for a sample of 179 APOGEE stars with high photometric quality and low interstellar extinction.

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