Examples of comparisons of Atlas9 model fluxes (black lines) with UV-spectrophotometry from the IUE satellite (gray lines) and with photometric measurements – UBV from Mermilliod & Mermilliod (1994), JHK from 2MASS – for two of our sample stars. The SEDs shown are dereddened according to the values of E(B − V) and R_V in Table 4, and normalised in V.