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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 (BV) (lower panel) estimates for each star. The solid lines are correction functions for specific (BV) indices.

This figure is made of several images, please see below:

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