Stellar Ages from Models using L, Teff

By applying the models used in Tetzlaff et al. 2011, I can obtain ages from Teff and luminosity, which will come from B-V data and spectral type. This is one way I can fill in the blanks in the age data for the DEBRIS catalog.Also, There is a table mentioned in Tetzlaff et al 2011 which lists many ages for young runaway stars.