We demonstrate an approach to determine spectral energy distribution (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. https://www.diegojavierfares.com/super-find-Frigorifico-combi-LG-GBB72MBUBN-No-frost-203-cm-Acero-antihuellas-texturizado-hot-choice/