Table 2.
Spectrometric properties for the VGS.
| Name | log10M⋆ | log10MH I | log10SFR | z | DL |
|---|---|---|---|---|---|
| [M⊙] | [M⊙] | [M⊙ yr−1] | [Mpc] | ||
| (1) | (2) | (3) | (4) | (5) | |
| VGS01 | 8.65 ± 0.10 | < 8.32 | −1.28 ± 0.11 | 0.019 | 80.5 |
| VGS02 | 8.65 ± 0.08 | 8.83 ± 0.12 | −1.57 ± 0.14 | 0.023 | 98.3 |
| VGS03 | 8.38 ± 0.09 | < 8.27 | −1.96 ± 0.12 | 0.017 | 73.2 |
| VGS04 | 8.87 ± 0.08 | < 8.23 | −1.13 ± 0.04 | 0.016 | 70.4 |
| VGS05 | 10.11 ± 0.09 | < 8.51 | −1.38 ± 0.29 | 0.022 | 97.7 |
| VGS06 | 8.42 ± 0.06 | 9.20 ± 0.07 | −1.17 ± 0.10 | 0.023 | 100.4 |
| VGS07 | 7.71 ± 0.19 | 8.93 ± 0.04 | −1.10 ± 0.03 | 0.016 | 70.5 |
| VGS08 | – | 8.60 ± 0.16 | −1.52 ± 0.13 | 0.020 | 85.3 |
| VGS09 | 7.85 ± 0.05 | 9.03 ± 0.04 | −1.43 ± 0.04 | 0.013 | 56.2 |
| VGS10 | 8.35 ± 0.06 | 9.17 ± 0.06 | −1.59 ± 0.02 | 0.016 | 68.4 |
| VGS11 | 9.06 ± 0.08 | 9.35 ± 0.04 | −2.05 ± 0.24 | 0.016 | 71.5 |
| VGS12 | 8.20 ± 0.05 | 9.48 ± 0.06 | −1.35 ± 0.13 | 0.018 | 77.3 |
| VGS13 | 9.03 ± 0.08 | 9.11 ± 0.08 | −1.14 ± 0.14 | 0.019 | 83.1 |
| VGS14 | 8.20 ± 0.06 | 8.81 ± 0.07 | −1.74 ± 0.07 | 0.013 | 56.9 |
| VGS15 | 9.41 ± 0.09 | – | −0.70 ± 0.32 | 0.019 | 82.9 |
| VGS16 | 7.93 ± 0.06 | < 8.06 | −2.10 ± 0.05 | 0.013 | 57.6 |
| VGS17 | – | – | −1.52 ± 0.09 | 0.011 | 46.2 |
| VGS18 | 8.32 ± 0.07 | 8.61 ± 0.12 | −2.70 ± 0.00 | 0.016 | 71.0 |
| VGS19 | 8.57 ± 0.08 | 8.50 ± 0.10 | −1.25 ± 0.09 | 0.014 | 62.6 |
| VGS20 | 7.66 ± 0.13 | – | −1.15 ± 0.06 | 0.017 | 72.1 |
| VGS21 | 9.97 ± 0.09 | 9.34 ± 0.07 | −0.64 ± 0.34 | 0.017 | 75.3 |
| VGS22 | 8.28 ± 0.06 | < 8.42 | −1.66 ± 0.06 | 0.019 | 83.3 |
| VGS23 | 9.28 ± 0.08 | 9.60 ± 0.05 | −0.98 ± 0.12 | 0.017 | 72.4 |
| VGS24 | 10.00 ± 0.10 | < 8.53 | −0.08 ± 0.43 | 0.023 | 101.2 |
| VGS25 | 8.14 ± 0.05 | 8.24 ± 0.16 | −0.95 ± 0.08 | 0.019 | 82.6 |
| VGS26 | 9.30 ± 0.11 | 9.18 ± 0.09 | −1.10 ± 0.16 | 0.023 | 101.1 |
| VGS27 | 7.98 ± 0.06 | 8.54 ± 0.09 | −2.22 ± 0.00 | 0.015 | 64.7 |
| VGS28 | – | < 8.22 | – | 0.015 | 66.2 |
| VGS29 | 8.91 ± 0.07 | – | −1.05 ± 0.14 | 0.020 | 87.1 |
| VGS30 | 8.00 ± 0.07 | 8.77 ± 0.07 | −2.30 ± 0.17 | 0.019 | 84.5 |
| VGS31 | 9.55 ± 0.09 | 9.31 ± 0.06 | 0.31 ± 0.00 | 0.021 | 91.0 |
| VGS32 | 9.44 ± 0.08 | 9.59 ± 0.05 | −0.64 ± 0.08 | 0.012 | 51.1 |
| VGS33 | 8.24 ± 0.07 | 8.93 ± 0.09 | – | 0.018 | 79.2 |
| VGS34 | 9.88 ± 0.10 | 9.39 ± 0.05 | – | 0.017 | 71.7 |
| VGS35 | 8.82 ± 0.08 | 9.03 ± 0.05 | −1.07 ± 0.16 | 0.017 | 75.1 |
| VGS36 | 8.95 ± 0.07 | 9.31 ± 0.06 | −0.80 ± 0.14 | 0.022 | 97.6 |
| VGS37 | 8.61 ± 0.07 | 9.13 ± 0.06 | −1.36 ± 0.11 | 0.019 | 84.1 |
| VGS38 | 7.86 ± 0.10 | 9.03 ± 0.03 | −1.30 ± 0.00 | 0.014 | 59.8 |
| VGS39 | 10.01 ± 0.10 | < 8.41 | −0.85 ± 0.16 | 0.019 | 82.7 |
| VGS40 | 9.07 ± 0.08 | 8.79 ± 0.10 | −0.73 ± 0.10 | 0.024 | 103.4 |
| VGS41 | 8.78 ± 0.08 | < 8.46 | −1.09 ± 0.12 | 0.023 | 101.9 |
| VGS42 | 9.40 ± 0.09 | 8.61 ± 0.16 | −0.82 ± 0.15 | 0.019 | 81.5 |
| VGS43 | 8.28 ± 0.07 | < 8.46 | −1.59 ± 0.13 | 0.021 | 93.4 |
| VGS44 | 9.51 ± 0.12 | 8.69 ± 0.10 | −0.21 ± 0.10 | 0.018 | 76.6 |
| VGS45 | 8.02 ± 0.06 | 8.55 ± 0.16 | −2.22 ± 0.00 | 0.015 | 63.0 |
| VGS46 | 8.51 ± 0.08 | 8.75 ± 0.13 | −1.35 ± 0.04 | 0.016 | 69.0 |
| VGS47 | 10.33 ± 0.09 | 9.12 ± 0.09 | −0.10 ± 0.18 | 0.022 | 96.5 |
| VGS48 | 9.29 ± 0.10 | – | −1.12 ± 0.19 | 0.025 | 109.0 |
| VGS49 | 9.52 ± 0.10 | < 8.56 | −0.22 ± 0.09 | 0.025 | 108.8 |
| VGS50 | 9.92 ± 0.09 | 9.74 ± 0.06 | −0.66 ± 0.16 | 0.020 | 88.6 |
| VGS51 | 8.55 ± 0.05 | 9.30 ± 0.05 | −0.31 ± 0.04 | 0.025 | 110.5 |
| VGS52 | 8.11 ± 0.07 | 8.95 ± 0.11 | −1.70 ± 0.20 | 0.018 | 78.2 |
| VGS53 | 9.50 ± 0.09 | 8.72 ± 0.14 | −0.64 ± 0.14 | 0.021 | 93.5 |
| VGS54 | 9.63 ± 0.09 | 9.55 ± 0.05 | −0.76 ± 0.12 | 0.024 | 104.2 |
| VGS55 | 9.20 ± 0.07 | 9.25 ± 0.09 | −0.83 ± 0.09 | 0.025 | 109.8 |
| VGS56 | 9.69 ± 0.10 | < 8.43 | −0.63 ± 0.16 | 0.019 | 81.3 |
| VGS57 | 10.06 ± 0.11 | 8.81 ± 0.10 | 0.23 ± 0.07 | 0.022 | 96.6 |
| VGS58 | 8.59 ± 0.06 | 8.87 ± 0.04 | −1.34 ± 0.08 | 0.012 | 49.8 |
| VGS59 | 8.26 ± 0.07 | < 8.41 | −1.85 ± 0.06 | 0.019 | 82.7 |
| VGS60 | 9.75 ± 0.09 | 8.41 ± 0.27 | −0.94 ± 0.12 | 0.020 | 85.4 |
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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