Comparison of single‐burst star formation models with the extinction‐corrected spectral energy distribution. The three models represent (from top to bottom): a 10 Myr single burst with E(B − V) = 0.3, a 200 Myr burst with E(B − V) = 0.18, and a 400 Myr burst with E(B − V) = 0. All models are scaled to match the optical data (1200–3000 Å rest), and the dashed lines connect the SED points with the same extinction correction. The 10 Myr model and data are shifted by +1 in the log for clarity.