Fig. 7
Upper panel: comparison between Hall (1996) and our calibration of near-IR continuum absolute fluxes. Lower panel: strong [Fe/H] correlation in the differences between the absolute continuum flux estimates. The colors are related to different [Fe/H] (upper panel) and (B−V) (lower panel) estimates for each star. The solid lines are correction functions for specific (B−V) indices.
This figure is made of several images, please see below:
