Reconstructions of the Main Sequence

The interpolated spectra used as inputs in computing the UBVRI magnitudes used in Figures 5 and 6 of the paper can be dowloaded from here:

spectra from this library spectra from this library with Predicted Lines included integrated fluxes from ODFNEW model atmospheres (1221 pt, Castelli & Kurucz 2003) integrated fluxes from NOVER model atmospheres (1221 pt, Castelli et al. 1997)