Comparison of the observed energy distribution from Adelman (filled black diamonds), TD1 (filled black squares) and 2MASS photometric data (filled red squares) with the best-fit theoretical flux (solid red line) calculated after five abundance analysis iterations for the LLMODELS atmosphere of HD 120198 with the parameters T_eff = 10173 K and logg = 4.2. Open blue diamonds show the theoretical fluxes convolved with the corresponding filters. The shaded area illustrates the spectral regions that were excluded from the fit.