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Fig. 2.

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Distribution of 3D half stellar mass radius (log Rhsm), SDSS (g − r) colour, stellar age in r band (log ager), and Sérsic index (nSérsic) versus stellar mass (log M*) for selected spheroidal galaxies (blue points), their massive sub-sample ( M > 10 11 M $ \mathrm{M}_* > 10^{11}\,\mathrm{M}_{\odot} $; orange points), and the full sample of galaxies (with M > 2 × 10 9 M $ \mathrm{M}_* > 2 \times 10^{9}\,\mathrm{M}_{\odot} $; black contours) from the HR5 simulations at z = 0.625, respectively. The dashed black line in the bottom right-hand panel indicates nSérsic = 1.5.

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