Comparison between the theoretical and observed spectrophotometry of HD 125248. The light gray curve shows the spectral energy distribution computed using a model atmosphere with T_eff = 9850 K, log g = 4.05, including the effects of individual nonsolar abundances of HD 125248 and a magnetic field with strength ⟨ B ⟩ = 7200 G. The observations cover the UV (blue lines), optical (red circles) and near-IR (green squares) spectral regions.