Fig. 3
Distribution of Sersic index (right panels) and effective radius (left panels) retrieved by GASPHOT for the spectroscopic members of our WINGS clusters in the three bands covered by our photometry: from top to bottom data are from the B images, the V images, and the K images. Dashed black lines refer to the entire WINGS sample, while the colored continuous lines are for the spectroscopic members observed in the three bands.
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