Table 1.
Photometric properties for the VGS.
Name | g | r | g − r | r25 | i( * ) |
---|---|---|---|---|---|
[mag] | [mag] | [mag] | [arcsec] | [°] | |
(1) | (2) | (3) | (4) | (5) | |
VGS01 | 17.87 | 17.42 | 0.45 | 9.8 | 60.0 |
VGS02 | 17.72 | 17.34 | 0.38 | 11.8 | 47.0 |
VGS03 | 17.86 | 17.43 | 0.43 | 8.4 | 55.0 |
VGS04 | 17.22 | 16.76 | 0.46 | 7.0 | 46.0 |
VGS05 | 15.68 | 14.94 | 0.74 | 23.0 | 37.0 |
VGS06 | 17.67 | 17.34 | 0.33 | 12.5 | 71.0 |
VGS07 | 17.45 | 17.38 | 0.07 | 11.2 | 50.0 |
VGS08 | 24.57 | 22.87 | 1.71 | 1.5 | 51.0 |
VGS09 | 17.71 | 17.48 | 0.23 | 19.4 | 68.0 |
VGS10 | 17.20 | 16.86 | 0.34 | 1.8 | 87.0 |
VGS11 | 16.44 | 15.98 | 0.46 | 19.9 | 18.0 |
VGS12 | 17.64 | 17.36 | 0.28 | 11.1 | 29.0 |
VGS13 | 16.77 | 16.30 | 0.47 | 14.4 | 68.0 |
VGS14 | 17.00 | 16.73 | 0.26 | 18.8 | 67.0 |
VGS15 | 15.85 | 15.30 | 0.55 | 31.9 | – |
VGS16 | 17.81 | 17.52 | 0.29 | 10.4 | 60.0 |
VGS17 | 20.97 | 21.09 | −0.12 | 1.8 | – |
VGS18 | 17.82 | 17.44 | 0.38 | 17.6 | 82.0 |
VGS19 | 16.89 | 16.50 | 0.39 | 9.0 | 60.0 |
VGS20 | 18.15 | 18.01 | 0.14 | 5.2 | – |
VGS21 | 15.49 | 14.81 | 0.69 | 43.8 | 79.0 |
VGS22 | 17.81 | 17.50 | 0.31 | 6.6 | 63.0 |
VGS23 | 15.53 | 15.14 | 0.38 | 22.4 | 49.0 |
VGS24 | 15.45 | 14.87 | 0.58 | 16.4 | 35.0 |
VGS25 | 17.83 | 17.60 | 0.23 | 9.7 | 43.0 |
VGS26 | 16.74 | 16.33 | 0.42 | 20.0 | 69.0 |
VGS27 | 18.04 | 17.72 | 0.32 | 9.1 | 55.0 |
VGS28 | 18.18 | 17.54 | 0.64 | 19.5 | 54.0 |
VGS29 | 16.60 | 16.23 | 0.38 | 15.6 | – |
VGS30 | 18.13 | 17.96 | 0.17 | 18.8 | 77.0 |
VGS31 | 15.01 | 14.70 | 0.31 | 15.5 | 52.0 |
VGS32 | 14.57 | 14.12 | 0.45 | 27.0 | 46.0 |
VGS33 | 17.97 | 17.61 | 0.37 | 8.9 | 60.0 |
VGS34 | 16.11 | 15.26 | 0.86 | 16.7 | 50.0 |
VGS35 | 16.74 | 16.33 | 0.41 | 13.2 | 65.0 |
VGS36 | 16.74 | 16.41 | 0.33 | 18.2 | 79.0 |
VGS37 | 17.38 | 17.04 | 0.34 | 23.1 | 67.0 |
VGS38 | 17.05 | 16.98 | 0.07 | 16.9 | 39.0 |
VGS39 | 16.00 | 15.21 | 0.79 | 15.4 | 66.0 |
VGS40 | 17.25 | 16.82 | 0.43 | 9.0 | 42.0 |
VGS41 | 17.60 | 17.19 | 0.41 | 6.2 | 29.0 |
VGS42 | 16.33 | 15.80 | 0.53 | 14.8 | 58.0 |
VGS43 | 18.16 | 17.83 | 0.33 | 7.3 | 30.0 |
VGS44 | 15.20 | 14.80 | 0.40 | 17.1 | 31.0 |
VGS45 | 17.61 | 17.35 | 0.26 | 20.8 | 66.0 |
VGS46 | 17.13 | 16.78 | 0.35 | 14.1 | 71.0 |
VGS47 | 15.23 | 14.51 | 0.71 | 29.5 | 72.0 |
VGS48 | 17.61 | 17.02 | 0.59 | 11.4 | – |
VGS49 | 15.85 | 15.46 | 0.39 | 12.3 | 40.0 |
VGS50 | 16.00 | 15.32 | 0.69 | 12.6 | 83.0 |
VGS51 | 17.25 | 17.03 | 0.22 | 12.8 | 63.0 |
VGS52 | 17.79 | 17.56 | 0.23 | 16.2 | 70.0 |
VGS53 | 16.12 | 15.61 | 0.50 | 20.5 | 64.0 |
VGS54 | 16.80 | 16.15 | 0.65 | 22.5 | 80.0 |
VGS55 | 16.63 | 16.19 | 0.44 | 18.1 | 55.0 |
VGS56 | 16.44 | 15.72 | 0.72 | 14.0 | 59.0 |
VGS57 | 14.94 | 14.44 | 0.50 | 21.5 | 30.0 |
VGS58 | 16.05 | 15.65 | 0.40 | 21.3 | 38.0 |
VGS59 | 18.12 | 17.76 | 0.36 | 12.7 | 67.0 |
VGS60 | 16.45 | 15.72 | 0.73 | 19.2 | 81.0 |
Notes. Columns (1) and (2) are the dereddened g and r-band magnitudes from SDSS. Column (3) is the dereddened g − r colour. Column (4) is the radius of the galaxy at isophote 25, calculated using the r-Petrosian R90 in the r band from SDSS as r25 = 1.7 × R90 (see Sect. 2.1.4). Column (5) is the galaxy inclination from Kreckel et al. (2012). ( * )We only need the inclination for galaxies observed in CO to calculate the aperture correction factor.
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