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


Table 4.

Spectrometric properties for the VGS companions.

Name log10M log10MH I log10SFR z DL
[M] [M] [M yr−1] [Mpc]
(1) (2) (3) (4) (5)
VGS07a 8.52 ± 0.09 0.016 70.5
VGS09a 7.79 ± 0.10 0.013 56.2
VGS10a 8.93 ± 0.10 0.016 68.4
VGS26a 10.31 ± 0.04 0.023 101.1
VGS30a 8.71 ± 0.07 0.019 84.5
VGS31a 10.02 ± 0.14 9.26 ± 0.05 0.81 ± 0.00 0.021 91.0
VGS31b 8.47 ± 0.05 8.45 ± 0.15 −0.82 ± 0.00 0.021 91.0
VGS34a 7.71 ± 0.13 0.017 71.7
VGS36a < 11.83 0.022 97.6
VGS37a 9.19 ± 0.05 −1.15 ± 0.07 0.019 84.1
VGS38a 7.65 ± 0.05 8.02 ± 0.06 −1.74 ± 0.07 0.014 59.8
VGS38b 8.21 ± 0.06 −2.30 ± 0.00 0.014 59.8
VGS39a 8.50 ± 0.05 0.019 82.7
VGS51a 8.37 ± 0.04 0.025 110.5
VGS53a 8.58 ± 0.25 0.021 93.5
VGS54a < 11.65 0.024 104.2
VGS56a 8.25 ± 0.16 0.019 81.3
VGS57a 8.00 ± 0.07 8.41 ± 0.08 0.022 96.6

Notes. Column (1) is the stellar mass from MPA-JHU (Kauffmann et al. 2003; Salim et al. 2007). Column (2) is the atomic gas mass from WSRT (Kreckel et al. 2012); it has been re-scaled to the luminosity distance in Col. (5). Column (3) is the Hα based SFR from Beygu et al. (2016). Column (4) is the redshift from MPA-JHU. Column (5) is the luminosity distance.

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