Absolute Calibration. IV. Use of G-type Stars as Primary Calibrators
We demonstrate an approach to determine spectral energy distribution royal fryer rft-50 (SED) templates that are accurate to the 1% level from the visible through the infrared for nearby (unextincted) solar-type stars.Our approach is based only on measurements of T _eff , log( g ), and M/H and the use of standard theoretical SED models.The success