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Fig. 13


Comparison between physical parameters (color excess, age, SFR, and stellar mass) derived with and without accounting for nebular emission, assuming a constant SFH and an SMC curve. Dashed lines show the one-to-one relations. The distribution for each parameter is shown at the top of each figure along the x-axis for parameters derived with nebular emission (blue histograms) and at the right side along the y-axis for parameters derived without nebular emission (red histograms). Typical error bars for each parameter are shown on the lower right side.

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