Spectral fit for N206-FS 187. The upper panel shows the model SED (red) fitted to the available photometry from optical (UBV and I) and infrared (JHK_s and IRAC 3.6 and 4.5 μm) bands (blue boxes) as well as the calibrated UV spectra from HST and IUE. The lower panels show the normalized HST and VLT-FLAMES spectra (blue solid line), overplotted with the PoWR model (red dashed line). The parameters of this best-fit model are given in Table 3. The observed spectrum also contains nebular emission lines (neb) and interstellar absorption lines (is).