Table 2
Photometric parameters for the sample of dEs.
| Galaxy | M V | ϵ V | R SMA,V | ⟨ μe,V ⟩ | M K | ϵ K | R SMA,K | ⟨ μe,K ⟩ | (V − K)e | Ref. |
| (mag) | (arcsec) | (mag arcsec-2) | (mag) | (arcsec) | (mag arcsec-2) | mag | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| VCC 21 | –16.75 ± 0.03 | 0.36 ± 0.03 | 13.86 ± 0.17 | 21.59 ± 0.06 | –18.47 ± 0.05 | 0.35 ± 0.02 | 10.80 ± 0.38 | 18.81 ± 0.10 | 2.42 ± 0.06 | 2 |
| VCC 308 | –17.65 ± 0.05 | 0.04 ± 0.03 | 19.16 ± 0.07 | 21.79 ± 0.04 | –19.79 ± 0.07 | 0.06 ± 0.03 | 16.70 ± 0.05 | 18.83 ± 0.06 | 2.79 ± 0.06 | 2 |
| VCC 397 | –16.44 ± 0.05 | 0.33 ± 0.03 | 13.56 ± 0.14 | 21.86 ± 0.05 | –18.96 ± 0.07 | 0.37 ± 0.04 | 13.05 ± 0.10 | 18.77 ± 0.09 | 3.08 ± 0.05 | 1 |
| VCC 523 | –18.23 ± 0.03 | 0.25 ± 0.01 | 26.73 ± 0.46 | 21.70 ± 0.05 | –20.59 ± 0.23 | 0.27 ± 0.02 | 17.34 ± 0.01 | 18.30 ± 0.23 | 2.91 ± 0.23 | 1 |
| VCC 856 | –17.45 ± 0.06 | 0.08 ± 0.03 | 16.21 ± 0.18 | 21.63 ± 0.05 | –19.67 ± 0.08 | 0.11 ± 0.05 | 14.15 ± 0.21 | 18.68 ± 0.09 | 2.86 ± 0.05 | 2 |
| VCC 917 | –16.26 ± 0.03 | 0.41 ± 0.02 | 9.68 ± 0.07 | 21.22 ± 0.05 | –18.42 ± 0.06 | 0.37 ± 0.07 | 8.61 ± 0.07 | 18.49 ± 0.13 | 2.80 ± 0.06 | 2 |
| VCC 990 | –17.13 ± 0.03 | 0.34 ± 0.02 | 9.88 ± 0.06 | 20.52 ± 0.04 | –19.58 ± 0.06 | 0.36 ± 0.04 | 10.49 ± 0.05 | 18.17 ± 0.09 | 2.92 ± 0.06 | 1 |
| VCC 1087 | –17.97 ± 0.06 | 0.28 ± 0.03 | 27.02 ± 0.29 | 21.94 ± 0.06 | –20.55 ± 0.16 | 0.32 ± 0.04 | 17.47 ± 0.09 | 18.57 ± 0.16 | 2.97 ± 0.15 | 1 |
| VCC 1122 | –16.86 ± 0.03 | 0.50 ± 0.04 | 14.26 ± 0.14 | 21.27 ± 0.10 | –18.98 ± 0.05 | 0.55 ± 0.08 | 11.81 ± 0.18 | 18.27 ± 0.20 | 2.82 ± 0.05 | 2 |
| VCC 1183 | –17.55 ± 0.03 | 0.22 ± 0.12 | 21.85 ± 0.28 | 21.99 ± 0.17 | –19.98 ± 0.05 | 0.31 ± 0.09 | 19.37 ± 0.42 | 18.80 ± 0.16 | 3.09 ± 0.05 | 2 |
| VCC 1261 | –18.38 ± 0.06 | 0.37 ± 0.05 | 23.76 ± 0.21 | 21.28 ± 0.08 | –20.94 ± 0.15 | 0.41 ± 0.06 | 20.37 ± 0.10 | 18.32 ± 0.18 | 2.80 ± 0.14 | 1 |
| VCC 1431 | –17.28 ± 0.06 | 0.03 ± 0.01 | 10.31 ± 0.05 | 20.78 ± 0.03 | –20.26 ± 0.16 | 0.02 ± 0.02 | 9.91 ± 0.08 | 17.73 ± 0.15 | 3.11 ± 0.15 | 1 |
| VCC 1549 | –16.96 ± 0.03 | 0.16 ± 0.01 | 13.09 ± 0.08 | 21.55 ± 0.03 | –19.43 ± 0.06 | 0.19 ± 0.01 | 11.83 ± 0.08 | 18.36 ± 0.06 | 3.10 ± 0.06 | 2 |
| VCC 1695 | –17.33 ± 0.08 | 0.22 ± 0.05 | 27.61 ± 0.73 | 22.69 ± 0.09 | –19.11 ± 0.13 | 0.16 ± 0.07 | 18.43 ± 0.06 | 19.24 ± 0.14 | 2.86 ± 0.10 | 2 |
| VCC 1861 | –17.55 ± 0.06 | 0.04 ± 0.02 | 21.57 ± 0.28 | 22.12 ± 0.04 | –20.60 ± 0.09 | 0.01 ± 0.01 | 20.11 ± 0.08 | 18.94 ± 0.07 | 3.21 ± 0.08 | 1 |
| VCC 1910 | –17.43 ± 0.06 | 0.14 ± 0.04 | 14.24 ± 0.11 | 21.20 ± 0.06 | –19.55 ± 0.08 | 0.17 ± 0.01 | 11.92 ± 0.04 | 18.65 ± 0.06 | 2.88 ± 0.06 | 1 |
| VCC 1912 | –17.58 ± 0.03 | 0.54 ± 0.06 | 23.53 ± 0.17 | 21.55 ± 0.15 | –20.18 ± 0.05 | 0.59 ± 0.08 | 21.14 ± 0.58 | 18.59 ± 0.23 | 2.77 ± 0.05 | 1 |
| VCC 1947 | –17.33 ± 0.03 | 0.23 ± 0.01 | 11.26 ± 0.08 | 20.76 ± 0.03 | –20.31 ± 0.12 | 0.23 ± 0.01 | 9.56 ± 0.05 | 17.42 ± 0.12 | 3.25 ± 0.12 | 1 |
Notes. Columns 2–5 present the absolute magnitude, the ellipticity, the half light radius along the semimajor axis, and the effective surface brightness within this effective radius in V band (Johnson-Cousins), respectively. Columns 6–9 show the same parameters in K band. All the magnitudes used throughout this work are referred to Vega. The transformation from this half light radius to the one used in the scaling relations, the geometric half light radius, is 
. Column 10 is the (V − K)e colour measured within an aperture with the size of the half light radius of each galaxy measured in the SDSS g band. Column 11 specifies the reference of the infrared image: 1 means this work (from H or K band photometry), 2 means that the image was gathered from GOLDMine database (H band, Gavazzi et al. 2003). The distances assumed for each galaxy are calculated from their surface brightness fluctuations by Mei et al. (2007), or similarly using H0 = 73 km s-1 Mpc-1, see Paper I for the list of individual distances.
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