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Table C.3

List of the derived parameters of all galaxies in our basic sample that are also parts of the galaxies provided in Taylor et al. (2010).

Taylor ID R r σ 0 μ r M r (Mg − Mr) M z log10(Mdyn) log10(M∗) ♈dyn ♈∗
[kpc] [km s-1] [] [mag] [mag] [mag] [log10(M⊙)] [log10(M⊙)] [M⊙/L⊙ ,r] [M⊙/L⊙ ,r]
55 2.76 ± 0.05 391± 12 18.80 ± 0.04 −22.08 ± 0.01 0.77 ± 0.01 −22.68 ± 0.01 11.69 ± 0.02 11.12 ± 0.15 9.39 ± 0.40 2.51 ± 1.04
49 1.32 ± 0.04 344± 15 17.50 ± 0.06 −21.79 ± 0.01 0.77 ± 0.01 −22.46 ± 0.01 11.26 ± 0.02 10.95 ± 0.15 4.54 ± 0.26 2.23 ± 0.92
62 2.71 ± 0.06 248± 11 18.81 ± 0.05 −22.05 ± 0.01 0.76 ± 0.01 −22.91 ± 0.01 11.29 ± 0.02 11.23 ± 0.15 3.84 ± 0.21 3.32 ± 1.37
30 1.72 ± 0.02 213± 9 17.99 ± 0.03 −21.87 ± 0.01 0.69 ± 0.01 −22.40 ± 0.01 10.96 ± 0.02 10.91 ± 0.15 2.12 ± 0.10 1.89 ± 0.78
21 1.51 ± 0.03 253± 8 18.29 ± 0.04 −21.27 ± 0.01 0.81 ± 0.01 −21.98 ± 0.01 11.05 ± 0.02 10.80 ± 0.15 4.57 ± 0.19 2.55 ± 1.05
38 1.04 ± 0.03 197± 10 17.15 ± 0.05 −21.62 ± 0.01 0.76 ± 0.01 −22.20 ± 0.01 10.67 ± 0.02 10.83 ± 0.15 1.38 ± 0.08 2.00 ± 0.83
19 1.66 ± 0.03 327± 13 18.54 ± 0.04 −21.22 ± 0.01 0.76 ± 0.01 −21.87 ± 0.01 11.31 ± 0.02 10.78 ± 0.15 8.76 ± 0.41 2.58 ± 1.07
22 1.72 ± 0.08 159± 16 18.62 ± 0.10 −21.25 ± 0.01 0.85 ± 0.02 −21.87 ± 0.02 10.70 ± 0.05 10.87 ± 0.15 2.09 ± 0.24 3.03 ± 1.25
18 1.84 ± 0.07 203± 14 18.90 ± 0.09 −21.10 ± 0.01 0.76 ± 0.02 −21.83 ± 0.01 10.94 ± 0.03 10.82 ± 0.15 4.18 ± 0.34 3.11 ± 1.28
15 1.62 ± 0.03 201± 7 18.33 ± 0.04 −21.37 ± 0.01 0.75 ± 0.01 −22.02 ± 0.01 10.88 ± 0.02 10.78 ± 0.15 2.84 ± 0.12 2.21 ± 0.91
14 1.61 ± 0.04 180± 8 18.39 ± 0.05 −21.31 ± 0.01 0.81 ± 0.01 −21.89 ± 0.01 10.78 ± 0.02 10.79 ± 0.15 2.38 ± 0.13 2.41 ± 1.00
1 1.45 ± 0.02 178± 6 17.71 ± 0.04 −21.76 ± 0.01 0.69 ± 0.01 −22.26 ± 0.01 10.73 ± 0.02 10.76 ± 0.15 1.38 ± 0.06 1.50 ± 0.62
42 1.79 ± 0.03 254± 9 18.34 ± 0.03 −21.59 ± 0.01 0.79 ± 0.01 −22.21 ± 0.01 11.13 ± 0.02 10.88 ± 0.15 4.07 ± 0.17 2.27 ± 0.94
8 1.30 ± 0.01 185± 7 17.72 ± 0.03 −21.51 ± 0.01 0.69 ± 0.01 −22.09 ± 0.01 10.71 ± 0.02 10.69 ± 0.15 1.69 ± 0.07 1.59 ± 0.66
27 2.23 ± 0.05 210± 9 18.85 ± 0.05 −21.56 ± 0.01 0.74 ± 0.01 −22.15 ± 0.01 11.06 ± 0.02 10.76 ± 0.15 3.54 ± 0.18 1.78 ± 0.74
48 2.03 ± 0.02 204± 8 18.31 ± 0.03 −21.88 ± 0.01 0.71 ± 0.01 −22.46 ± 0.01 10.99 ± 0.02 11.01 ± 0.15 2.28 ± 0.10 2.36 ± 0.98
20 1.55 ± 0.03 276± 11 18.30 ± 0.04 −21.31 ± 0.01 0.80 ± 0.01 −21.91 ± 0.01 11.14 ± 0.02 10.79 ± 0.15 5.32 ± 0.26 2.39 ± 0.99
36 1.84 ± 0.03 242± 9 18.56 ± 0.04 −21.42 ± 0.01 0.80 ± 0.01 −22.12 ± 0.01 11.10 ± 0.02 10.89 ± 0.15 4.40 ± 0.20 2.72 ± 1.12
33 1.80 ± 0.03 286± 10 18.53 ± 0.04 −21.43 ± 0.01 0.80 ± 0.01 −22.04 ± 0.01 11.23 ± 0.02 10.83 ± 0.15 6.02 ± 0.26 2.39 ± 0.99
47 1.85 ± 0.02 190± 5 17.74 ± 0.02 −22.24 ± 0.00 0.70 ± 0.01 −22.74 ± 0.01 10.89 ± 0.01 10.97 ± 0.15 1.30 ± 0.04 1.56 ± 0.64
9 1.38 ± 0.02 259± 7 18.15 ± 0.03 −21.20 ± 0.01 0.77 ± 0.01 −21.84 ± 0.01 11.03 ± 0.01 10.74 ± 0.15 4.67 ± 0.16 2.38 ± 0.98
26 2.07 ± 0.06 209± 11 18.81 ± 0.06 −21.46 ± 0.01 0.76 ± 0.01 −22.08 ± 0.01 11.02 ± 0.02 10.84 ± 0.15 3.59 ± 0.22 2.38 ± 0.98
24 2.13 ± 0.05 183± 8 18.74 ± 0.05 −21.57 ± 0.01 0.74 ± 0.01 −22.15 ± 0.01 10.92 ± 0.02 10.85 ± 0.15 2.56 ± 0.13 2.18 ± 0.90
12 1.54 ± 0.03 160± 9 18.06 ± 0.04 −21.55 ± 0.01 0.69 ± 0.01 −22.13 ± 0.01 10.66 ± 0.03 10.68 ± 0.15 1.42 ± 0.09 1.51 ± 0.62
37 2.09 ± 0.08 225± 13 18.91 ± 0.08 −21.38 ± 0.01 0.82 ± 0.02 −22.07 ± 0.02 11.09 ± 0.03 10.89 ± 0.15 4.50 ± 0.32 2.81 ± 1.16
57 3.76 ± 0.12 139± 10 19.96 ± 0.07 −21.61 ± 0.01 0.67 ± 0.01 −22.20 ± 0.01 10.92 ± 0.03 10.84 ± 0.15 2.50 ± 0.20 2.06 ± 0.85
45 1.90 ± 0.04 244± 12 18.52 ± 0.05 −21.56 ± 0.01 0.81 ± 0.01 −22.16 ± 0.01 11.12 ± 0.02 10.98 ± 0.15 4.11 ± 0.24 2.95 ± 1.22
61 3.31 ± 0.03 299± 7 18.83 ± 0.02 −22.42 ± 0.01 1.05 ± 0.01 −23.02 ± 0.01 11.54 ± 0.01 11.19 ± 0.15 4.83 ± 0.14 2.19 ± 0.90
50 3.64 ± 0.09 187± 16 19.75 ± 0.05 −21.74 ± 0.01 0.77 ± 0.01 −22.18 ± 0.01 11.17 ± 0.04 10.83 ± 0.15 3.86 ± 0.35 1.78 ± 0.74
34 1.89 ± 0.03 218± 9 18.78 ± 0.03 −21.26 ± 0.01 0.79 ± 0.01 −21.89 ± 0.01 11.02 ± 0.02 10.83 ± 0.15 4.29 ± 0.20 2.74 ± 1.13
56 3.74 ± 0.03 252± 7 19.37 ± 0.02 −22.14 ± 0.01 0.81 ± 0.01 −22.71 ± 0.01 11.44 ± 0.01 11.12 ± 0.15 5.00 ± 0.15 2.37 ± 0.98
39 1.89 ± 0.04 202± 8 18.24 ± 0.04 −21.81 ± 0.01 0.69 ± 0.01 −22.38 ± 0.01 10.95 ± 0.02 10.90 ± 0.15 2.19 ± 0.10 1.93 ± 0.80
35 0.89 ± 0.02 383± 15 16.94 ± 0.05 −21.50 ± 0.01 0.80 ± 0.01 −22.20 ± 0.01 11.18 ± 0.02 10.87 ± 0.15 4.96 ± 0.25 2.45 ± 1.01
11 2.00 ± 0.06 166± 9 19.22 ± 0.06 −20.95 ± 0.01 0.71 ± 0.01 −21.56 ± 0.02 10.81 ± 0.03 10.53 ± 0.15 3.51 ± 0.23 1.86 ± 0.77
52 2.22 ± 0.03 270± 9 18.60 ± 0.03 −21.80 ± 0.01 0.83 ± 0.01 −22.43 ± 0.01 11.27 ± 0.02 10.99 ± 0.15 4.67 ± 0.19 2.45 ± 1.01
41 1.81 ± 0.03 181± 6 18.11 ± 0.04 −21.87 ± 0.01 0.72 ± 0.01 −22.47 ± 0.01 10.84 ± 0.02 10.87 ± 0.15 1.62 ± 0.07 1.75 ± 0.72
54 2.18 ± 0.02 339± 7 18.14 ± 0.02 −22.21 ± 0.01 0.76 ± 0.01 −22.87 ± 0.01 11.46 ± 0.01 11.12 ± 0.15 4.97 ± 0.14 2.25 ± 0.93
43 2.12 ± 0.05 238± 13 18.78 ± 0.05 −21.52 ± 0.01 0.77 ± 0.01 −22.15 ± 0.01 11.14 ± 0.02 10.88 ± 0.15 4.47 ± 0.27 2.42 ± 1.00
63 3.34 ± 0.05 310± 9 18.85 ± 0.03 −22.42 ± 0.01 0.80 ± 0.01 −23.08 ± 0.01 11.57 ± 0.01 11.30 ± 0.15 5.22 ± 0.18 2.80 ± 1.15
10 1.78 ± 0.03 168± 6 18.60 ± 0.03 −21.31 ± 0.01 0.78 ± 0.01 −21.90 ± 0.01 10.77 ± 0.02 10.80 ± 0.15 2.30 ± 0.10 2.49 ± 1.03
3 1.42 ± 0.02 218± 7 18.06 ± 0.04 −21.37 ± 0.01 0.74 ± 0.01 −21.94 ± 0.01 10.89 ± 0.02 10.71 ± 0.15 2.88 ± 0.11 1.92 ± 0.79
17 1.71 ± 0.03 322± 17 18.64 ± 0.04 −21.19 ± 0.01 0.82 ± 0.01 −21.89 ± 0.01 11.31 ± 0.02 10.82 ± 0.15 9.00 ± 0.54 2.88 ± 1.19
53 2.39 ± 0.04 280± 9 18.70 ± 0.03 −21.87 ± 0.01 0.79 ± 0.01 −22.50 ± 0.01 11.34 ± 0.02 11.05 ± 0.15 5.08 ± 0.20 2.60 ± 1.07
59 2.17 ± 0.02 368± 9 18.22 ± 0.02 −22.10 ± 0.01 0.84 ± 0.01 −22.80 ± 0.01 11.53 ± 0.01 11.10 ± 0.15 6.43 ± 0.19 2.37 ± 0.98
13 1.57 ± 0.03 361± 12 18.30 ± 0.03 −21.33 ± 0.01 0.76 ± 0.01 −21.91 ± 0.01 11.38 ± 0.02 10.85 ± 0.15 9.11 ± 0.39 2.70 ± 1.12
46 2.01 ± 0.07 224± 12 19.33 ± 0.07 −20.85 ± 0.01 0.86 ± 0.02 −21.65 ± 0.01 11.07 ± 0.03 10.83 ± 0.15 6.97 ± 0.47 4.04 ± 1.67
31 2.21 ± 0.05 182± 8 19.00 ± 0.05 −21.39 ± 0.01 0.71 ± 0.01 −22.01 ± 0.01 10.93 ± 0.02 10.75 ± 0.15 3.10 ± 0.17 2.05 ± 0.85
5 1.28 ± 0.04 197± 12 18.26 ± 0.06 −20.95 ± 0.01 0.75 ± 0.01 −21.78 ± 0.01 10.76 ± 0.03 10.57 ± 0.15 3.13 ± 0.22 2.01 ± 0.83
2 1.63 ± 0.03 209 ± 7 18.54 ± 0.04 −21.16 ± 0.01 0.74 ± 0.01 −21.82 ± 0.01 10.92 ± 0.02 10.72 ± 0.15 3.72 ± 0.16 2.35 ± 0.97
23 1.71 ± 0.02 154 ± 6 18.04 ± 0.02 −21.77 ± 0.00 0.67 ± 0.01 −22.29 ± 0.01 10.68 ± 0.02 10.77 ± 0.15 1.21 ± 0.05 1.52 ± 0.63
7 1.32 ± 0.02 172 ± 8 17.84 ± 0.04 −21.44 ± 0.01 0.70 ± 0.01 −22.12 ± 0.01 10.66 ± 0.02 10.78 ± 0.15 1.58 ± 0.08 2.09 ± 0.86
60 2.13 ± 0.02 290 ± 6 17.73 ± 0.02 −22.55 ± 0.00 0.74 ± 0.01 −23.23 ± 0.01 11.32 ± 0.01 11.02 ± 0.15 2.59 ± 0.07 1.29 ± 0.53
6 1.33 ± 0.03 174 ± 7 17.48 ± 0.05 −21.83 ± 0.01 0.69 ± 0.01 −22.38 ± 0.01 10.67 ± 0.02 10.84 ± 0.15 1.13 ± 0.05 1.66 ± 0.68
25 1.66 ± 0.03 235 ± 10 18.29 ± 0.04 −21.47 ± 0.01 0.78 ± 0.01 −22.07 ± 0.01 11.03 ± 0.02 10.81 ± 0.15 3.58 ± 0.17 2.17 ± 0.90
4 1.50 ± 0.04 220 ± 9 18.44 ± 0.05 −21.09 ± 0.01 0.77 ± 0.01 −21.74 ± 0.01 10.93 ± 0.02 10.69 ± 0.15 4.02 ± 0.20 2.34 ± 0.97
28 1.20 ± 0.02 206 ± 6 17.08 ± 0.03 −21.99 ± 0.01 0.67 ± 0.01 −22.54 ± 0.01 10.77 ± 0.01 10.84 ± 0.15 1.24 ± 0.04 1.46 ± 0.60
29 1.10 ± 0.03 297 ± 16 17.54 ± 0.06 −21.37 ± 0.01 0.83 ± 0.02 −22.06 ± 0.02 11.05 ± 0.02 10.88 ± 0.15 4.20 ± 0.26 2.83 ± 1.17
51 2.62 ± 0.06 227 ± 12 19.08 ± 0.05 −21.70 ± 0.01 0.82 ± 0.01 −22.26 ± 0.01 11.19 ± 0.02 10.93 ± 0.15 4.29 ± 0.26 2.31 ± 0.95
58 2.52 ± 0.03 253 ± 5 18.02 ± 0.03 −22.64 ± 0.00 0.70 ± 0.01 −23.22 ± 0.01 11.27 ± 0.01 11.18 ± 0.15 2.15 ± 0.06 1.74 ± 0.72
40 1.49 ± 0.02 229 ± 6 17.58 ± 0.03 −21.95 ± 0.00 0.72 ± 0.01 −22.54 ± 0.01 10.96 ± 0.01 10.88 ± 0.15 1.97 ± 0.06 1.65 ± 0.68

Notes.First column: IDs used in the table in their paper. Second column: scale radius Rr of the galaxies measured in the SDSS r band (in kpc). Third column: corrected central velocity dispersion σ0 (in km s-1). Fourth column: surface brightness μr measured in the SDSS r band (in mag/arcsec2). Fifth column: absolute magnitude in r band Mr. Sixth column: g − r colour (Mg − Mr) (in mag). Seventh column: logarithm of the dynamical mass Mdyn (in solar masses). Eighth column: logarithm of the stellar mass M* (in solar masses). Ninth column: dynamical mass-to-light ratio ♈dyn (in solar units M⊙/L⊙ ,r). Tenth column: stellar mass-to-light ratio ♈∗ (in solar units M⊙/L⊙ ,r).

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