Table B.1.
Summary of the metallicity of the total number of stars in the first 2 kpc of every halo.
Halos | N*2kpc | (-2< [Fe/H]<0) | (-4< [Fe/H]< -2) | (-6< [Fe/H]< -4) | (-8< [Fe/H]< -6) |
---|---|---|---|---|---|
% | % | % | % | ||
ψDMG1 | 12340 | 93.12 | 4.91 | 0.71 | 1.26 |
ψDMG2 | 1950 | 80.62 | 14.82 | 1.44 | 3.12 |
ψDMG3 | 1550 | 77.22 | 16.91 | 1.68 | 4.19 |
CDMG1 | 21206 | 95.62 | 3.61 | 0.36 | 0.41 |
CDMG2 | 7572 | 88.55 | 9.17 | 1.12 | 1.16 |
CDMG3 | 3417 | 83.79 | 12.38 | 1.82 | 2.01 |
“WDM”G1 | 28328 | 89.48 | 8.43 | 0.76 | 1.33 |
“WDM”G2 | 3793 | 79.25 | 14.79 | 2.14 | 3.82 |
“WDM”G3 | 5122 | 78.21 | 16.34 | 1.44 | 4.01 |
Notes. Column 1: Simulated Dwarf individual name, Column 2: Number of stars inside the first 2kpc N*2kpc, Column 3: Percentage of stars in column 2 with a [Fe/H] between 0 and -2, Column 4: Percentage of stars in column 2 with a [Fe/H] between -2 and -4, Column 5: Percentage of stars in column 2 with a [Fe/H] between -4 and -6, Column 6: Percentage of stars in column 2 with a [Fe/H] between -6 and -8. Data for halos at z = 5.56.
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