MIDIS - Near-infrared rest-frame morphology of massive galaxies at 3 < z < 5 in the Hubble eXtreme Deep Field

Open Access

Fig. 2.

Gini-M₂₀ diagram. The orange stars and green dots correspond to the nonparametric morphology measured on MIRI F560W and WFC3 F160W images, respectively. For each galaxy, gray lines link the observed morphology at different wavelengths. The ETGs, LTGs, and mergers are separated according to Eqs. (4) in Lotz et al. (2008).

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