Table 1.
Characteristics of the galaxies of our sample.
Label | Auriga | Stellar mass | DM mass | R200 | Rh | Macc |
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---|---|---|---|---|---|---|---|---|
[M⊙] | [M⊙] | [kpc] | [kpc] | [M⊙] | > 4 Rh | > 5 Rh | ||
1 | L5 | 2.08 × 1010 | 3.73 × 1011 | 138.179 | 7.736 | 1.08 × 109 | 0.24 | 0.37 |
2 | L1 | 1.81 × 1010 | 2.76 × 1011 | 125.475 | 5.394 | 3.45 × 109 | 0.61 | 0.67 |
3 | L4 | 1.80 × 1010 | 3.44 × 1011 | 138.676 | 6.793 | 1.77 × 109 | 0.39 | 0.49 |
4 | L3 | 1.78 × 1010 | 3.15 × 1011 | 129.183 | 5.554 | 1.10 × 109 | 0.34 | 0.50 |
5 | L7 | 1.23 × 1010 | 1.98 × 1011 | 114.386 | 5.032 | 1.19 × 109 | 0.45 | 0.54 |
6 | L0 | 8.83 × 109 | 1.36 × 1011 | 98.366 | 1.180 | 2.14 × 107 | 0.01 | 0.01 |
7 | L2 | 8.29 × 109 | 1.76 × 1011 | 108.487 | 7.050 | 3.44 × 108 | 0.53 | 0.69 |
8 | L6 | 7.89 × 109 | 1.15 × 1011 | 96.061 | 4.802 | 2.37 × 108 | 0.32 | 0.47 |
9 | L11 | 7.02 × 109 | 1.16 × 1011 | 94.728 | 4.544 | 5.11 × 108 | 0.31 | 0.38 |
10 | L9 | 6.30 × 109 | 1.24 × 1011 | 98.478 | 3.938 | 2.93 × 109 | 0.18 | 0.17 |
11 | L10 | 5.34 × 109 | 1.02 × 1011 | 92.078 | 3.314 | 7.71 × 107 | 0.07 | 0.11 |
12 | L8 | 5.09 × 109 | 1.37 × 1011 | 100.823 | 5.540 | 1.09 × 109 | 0.43 | 0.50 |
13 | LL2 | 3.46 × 109 | 6.10 × 1010 | 76.679 | 3.063 | 1.12 × 107 | 0.02 | 0.03 |
14 | LL9 | 1.06 × 109 | 4.44 × 1010 | 70.103 | 3.500 | 1.66 × 107 | 0.04 | 0.10 |
15 | LL8 | 4.54 × 108 | 1.55 × 1010 | 49.224 | 1.034 | 9.74 × 104 | 0.00 | 0.00 |
16 | LL6 | 4.53 × 108 | 3.66 × 1010 | 61.001 | 1.923 | 2.70 × 106 | 0.01 | 0.01 |
17 | LL11 | 3.28 × 108 | 3.06 × 1010 | 62.116 | 3.161 | 6.40 × 106 | 0.04 | 0.06 |
Notes. The galaxies are listed in order of decreasing stellar mass. The columns indicate: (1): label used in this work, (2): Auriga ID in Grand et al. (2024), (3): stellar mass, (4): DM mass, (5): R200, (6): half-light radius, (7): accreted stellar mass, (8): accreted mass fraction of the stellar halo (inner limit of 4 Rh, see Sect. 2.4); and (9) accreted mass fraction of the stellar halo but considering an inner limit of 5 Rh. An ‘L’ or ‘LL’ is added to the Auriga ID to distinguish DM halo masses of 1011 M⊙ and 1010 M⊙, respectively.
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