A semi-empirical absolute flux calibration in the near infrared: Direct stellar diameters vs. IRFM determinations
A new semi-empirical method to derive the absolute flux calibration in the near infrared (J,K,L and L' bands) is proposed. The method consists of the application of the InfraRed Flux Method (IRFM) to a selected sample of stars with accurate direst measurements of their angular diameters. The absolute fluxes in each band are obtained minimizing the
Alonso, A. et al.
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1994