Table 2.
Global properties of the 19 halos simulated when only Pop II stars are considered.
| Halo ID | LV | M⋆ | M200 | R200 | r1/2 | σLOS | [Fe/H] |
|---|---|---|---|---|---|---|---|
| [105 L⊙] | [105 L⊙] | [109 M⊙] | [kpc] | [kpc] | [km s−1] | [dex] | |
| h177 | 3.07 | 10.28 | 0.51 | 25.9 | 0.26 | 5.7 | −1.97 |
| h063 | 1.41 | 3.73 | 2.41 | 41.8 | 0.51 | 6.4 | −2.31 |
| h190 | 1.31 | 3.62 | 0.47 | 24.2 | 0.28 | 4.8 | −2.15 |
| h187 | 1.04 | 2.86 | 0.43 | 23.4 | 0.25 | 5.3 | −2.27 |
| h166 | 0.71 | 1.92 | 0.64 | 26.9 | 0.22 | 5.0 | −2.36 |
| h112 | 0.63 | 1.68 | 1.18 | 32.9 | 0.43 | 6.9 | −2.79 |
| h152 | 0.53 | 1.42 | 0.80 | 28.9 | 0.38 | 6.4 | −2.82 |
| h113 | 0.41 | 1.08 | 1.14 | 32.5 | 0.53 | 7.4 | −3.07 |
| h184 | 0.30 | 0.81 | 0.61 | 26.4 | 0.28 | 4.8 | −2.69 |
| h245 | 0.17 | 0.45 | 0.39 | 22.7 | 0.32 | 6.0 | −3.24 |
| h259 | 0.20 | 0.53 | 0.39 | 22.7 | 0.21 | 5.1 | −2.74 |
| h226 | 0.15 | 0.38 | 0.44 | 23.6 | 0.25 | 4.8 | −2.87 |
| h277 | 0.10 | 0.26 | 0.36 | 22.2 | 0.42 | 5.3 | −3.03 |
| h249 | 0.07 | 0.18 | 0.39 | 22.8 | 0.28 | 5.7 | −3.18 |
| h315 | 0.05 | 0.14 | 0.33 | 21.6 | 0.51 | 5.6 | −3.16 |
| h323 | 0.05 | 0.13 | 0.27 | 20.1 | 0.21 | 4.0 | −3.07 |
| h170 | 0.05 | 0.13 | 0.62 | 26.5 | 0.41 | 5.0 | −3.56 |
| h273 | 0.04 | 0.09 | 0.39 | 22.7 | 0.32 | 4.1 | −3.53 |
| h291 | 0.02 | 0.04 | 0.33 | 21.4 | 0.18 | 5.5 | −3.69 |
Notes. The first column gives the halo ID following Revaz & Jablonka (2018). LV is the V-band luminosity and M⋆ the stellar mass. M200 is the virial mass, i.e., the mass inside the virial radius R200. r1/2 is the half-light radius, σLOS is the line-of-sight velocity dispersion, and [Fe/H] is the peak value of the metallicity distribution function.
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