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This article has an erratum: [https://doi.org/10.1051/0004-6361/202141888e]


Table 3.

Photometric properties for the VGS companions.

Name g r g − r r25 i( * )
[mag] [mag] [mag] [arcsec] [°]
(1) (2) (3) (4) (5)
VGS07a 21.48 21.91 −0.43 8.5
VGS09a 23.46 23.52 −0.06 2.2
VGS10a 22.11 21.77 0.33 2.2
VGS26a 14.16 13.67 0.49 38.5
VGS30a 18.67 18.41 0.26 16.7
VGS31a 14.73 14.25 0.48 30.1 60.0
VGS31b 16.93 16.74 0.19 10.8
VGS34a 20.38 20.28 0.10 5.6
VGS36a 19.88 19.88 −0.00 2.5
VGS37a 16.57 16.22 0.35 16.9
VGS38a 17.69 17.57 0.13 7.8
VGS38b 19.03 18.86 0.17 9.8
VGS39a 19.39 19.44 −0.05 6.7
VGS51a 22.28 20.70 1.58 5.5
VGS53a 17.61 16.65 0.96 19.1
VGS54a 19.32 18.98 0.34 11.2
VGS56a 19.19 18.90 0.29 7.9
VGS57a 17.85 17.75 0.10 7.7

Notes. Columns (1) and (2) are the dereddened g and r-band magnitudes from SDSS derived in the same aperture. Column (3) is the dereddened g − r colour magnitude from SDSS. 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 HyperLEDA; there is no inclination data for VGS companions in Kreckel et al. (2012). ( * )We only need the inclination for galaxies observed in CO to calculate the aperture correction factor.

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