Table 1
Main characteristics of our subsample of the 15 most massive objects in S230A.
| Galaxy | N dark | N star | N gas | R 200 | M 200 | M star | M bar | n | R d | D / T |
| (kpc h-1) | (1011 M⊙h-1) | (1010 M⊙h-1) | (1010 M⊙h-1) | (kpc h-1) | ||||||
|
|
||||||||||
| G1 | 437 013 | 255 241 | 192 495 | 231.1 | 25.9 | 7.7 | 8.0 | 1.1 | 4.1 | 0.56 |
| G2 | 156 183 | 92 670 | 28 190 | 162.2 | 9.3 | 3.1 | 3.3 | 2.2 | 2.5 | 0.55 |
| G3 | 228 052 | 120 262 | 82 041 | 185.2 | 13.5 | 4.0 | 4.3 | 1.5 | 3.2 | 0.46 |
| G4 | 162 563 | 72 102 | 44 930 | 164.6 | 9.6 | 2.3 | 2.4 | 1.4 | 2.1 | 0.71 |
| G5 | 71 815 | 48 399 | 14 528 | 125.5 | 4.3 | 1.8 | 1.8 | 1.3 | 1.5 | 0.34 |
| G6 | 181 662 | 113 855 | 52 922 | 171.6 | 10.8 | 3.9 | 4.3 | 1.9 | 3.1 | 0.56 |
| G7 | 117 001 | 60 969 | 49 564 | 148.6 | 6.9 | 2.1 | 2.4 | 1.3 | 5.1 | 0.44 |
| G8 | 82 096 | 40 720 | 23 221 | 131.1 | 4.9 | 1.4 | 1.7 | 1.3 | 5.6 | 0.39 |
| G9 | 69 753 | 31 088 | 15 567 | 123.8 | 4.1 | 1.1 | 1.5 | 1.3 | 4.0 | 0.52 |
| G10 | 260 771 | 154 477 | 74 724 | 193.2 | 15.5 | 5.0 | 5.3 | 1.3 | 4.2 | 0.47 |
| G11 | 136 695 | 71 156 | 28 907 | 155.1 | 8.1 | 2.4 | 2.5 | 1.4 | 1.9 | 0.59 |
| G12 | 117 048 | 49 347 | 27 641 | 147.1 | 6.9 | 1.4 | 1.5 | 1.1 | 2.8 | 0.50 |
| G13 | 129 747 | 71 671 | 36 577 | 153.0 | 7.7 | 2.6 | 2.7 | 1.5 | 1.7 | 0.66 |
| G14 | 62 344 | 27 559 | 14 604 | 119.2 | 3.7 | 0.9 | 1.0 | 1.3 | 3.5 | 0.49 |
| G15 | 49 406 | 24 659 | 7370 | 110.0 | 2.9 | 0.8 | 0.9 | 1.3 | 1.4 | 0.27 |
Notes. Columns: number of dark matter (Ndark), star (Nstar), and gas (Ngas) particles within the virial radius, virial radius (R200), virial mass (M200), stellar (Mstar) and baryonic (Mbar) masses within the baryonic radius, Sérsic index for the central spheroid (n), disc scale length (Rd), and disc-to-total-mass ratio (D/T).
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