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Fig. 16.

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Optical (triangle and smaller star markers) and near-IR (circle and larger star markers) half-light radius measured in the closest band to 550 nm and 1.6 μm rest-frame, respectively, versus the total M* of the galaxy. Circular and triangular markers are individual galaxies, star markers are the mean value for each Type of galaxy with their associated error bar indicating the error of the mean. For each individual galaxy, we link their optical (triangles) and NIR sizes (circles) by a dashed line to illustrates the size evolution. The yellow and orange shaded regions illustrate the mass-size relation derived by van der Wel et al. (2014) in the optical bands and at the redshift of our sample.

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