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Table 1.

Main properties of the 28 CIELO galaxies analyzed.

Simulation ID Gal ropt rvir M⋆, gal M , halo T $ \mathrm{M}^{\mathrm{T}}_{\star, \mathrm{halo}} $ M⋆, halo Mvir
[kpc] [kpc] [M] [M] [M] [M]
LG1 4337 7.08 159.99 5.14e+10 1.96e+10 8.09e+09 1.37e+12
LG1 4469 7.33 137.02 8.06e+09 2.92e+09 1.03e+09 5.39e+11
LG1 2097 5.94 102.49 4.70e+09 1.82e+09 5.89e+08 2.25e+11
LG1 0000 11.35 109.50 4.60e+09 8.91e+08 1.64e+08 1.76e+11
LG1 0053 9.60 94.29 4.36e+09 2.19e+09 4.82e+08 1.66e+11
LG1 2177 6.54 85.46 3.61e+09 3.02e+09 4.29e+08 2.09e+11
LG1 2250 5.78 121.94 3.36e+09 8.90e+08 2.23e+08 7.59e+10
LG1 2208 5.83 79.62 2.51e+09 1.16e+09 1.79e+08 1.59e+11
LG1 4628 4.29 75.44 2.44e+09 9.20e+08 1.63e+08 1.24e+11
LG2 0190 8.53 115.24 1.46e+10 7.35e+09 1.61e+09 5.08e+11
P2 0214 9.57 85.67 7.22e+09 2.80e+09 3.83e+08 1.99e+11
P2 0272 5.79 61.46 1.58e+09 6.90e+08 2.01e+08 7.77e+10
P3 0232 5.89 96.77 1.65e+10 6.57e+09 1.16e+09 2.84e+11
P3 0271 8.89 88.11 3.29e+09 1.70e+09 3.51e+08 1.19e+11
P3 0875 9.80 75.83 2.87e+09 1.39e+09 2.33e+08 1.06e+11
P3 0000 11.19 82.66 1.92e+09 1.17e+09 2.55e+08 5.05e+10
P4 0349 7.60 110.63 1.84e+10 5.31e+09 1.60e+09 3.16e+11
P4 0000 4.77 88.18 1.32e+10 3.96e+09 5.05e+08 2.14e+11
P4 0428 7.02 98.71 1.24e+10 2.45e+09 7.17e+08 2.79e+11
P4 1248 9.92 103.27 5.86e+09 2.72e+09 6.64e+08 9.51e+10
P4 1266 9.19 86.79 3.12e+09 1.73e+09 3.38e+08 8.93e+10
P4 0018 4.06 69.36 1.90e+09 8.13e+08 2.20e+08 9.21e+10
P7 2389 10.25 146.55 5.43e+10 1.94e+10 5.26e+09 7.99e+11
P7 7805 10.93 146.54 4.09e+10 2.10e+10 6.79e+09 9.71e+11
P7 8958 7.16 91.51 1.48e+10 4.38e+09 1.59e+09 2.19e+11
P7 0000 6.35 93.28 5.38e+09 1.77e+09 4.18e+08 1.09e+11
P7 2627 9.43 71.73 4.69e+09 1.41e+09 2.49e+08 1.19e+11
P7 2696 2.82 58.28 2.30e+09 1.14e+09 2.01e+08 4.59e+10

Notes. From left to right: Simulation code, ID galaxies, ropt is the characteristic radius that encloses 83 percent of the stellar mass of the galaxy, M⋆, gal is the galaxy stellar mass up to 2ropt, rvir is the virial radius, M , halo T $ \mathrm{M}^{\mathrm{T}}_{\star, \mathrm{halo}} $ is the stellar halo mass up to virial radius, M⋆, halo is the stellar halo mass ranging from 1.5ropt to rvir, and Mvir is the mass of dark matter within the virial radius.

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