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

Open Access

Fig. 3.

Gini-M₂₀ diagram based on MIRI F560W morphology, separating galaxies at 3<z<3.75 with log(M_⋆/M_⊙)<9.5 (low-z/low-M_⋆; blue dots and shaded region), galaxies at 3<z<3.75 with log(M_⋆/M_⊙)>9.5 (low-z/high-M_⋆; green stars and shaded region), and galaxies at 3.75<z<5 (high-z/all-M_⋆; red squares and shaded region). ETGs, LTGs, and mergers are separated according to Eqs. (4) in Lotz et al. (2008).

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