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Table 1:

Principle properties of the sample of 35 galaxies used in this study, in order of increasing RA (see Sect. 2.5).
IAU ID z D.C. $V_{\rm flat}$ $\Delta V_{\rm flat}$ $\log{(M_{\rm stellar}/M_\odot)}$ ${\it SFR}_{\rm UV}$ ${\it SFR}_{\rm IR}$ ${\it SFR}$ $\Delta {\it SFR}$ $R_{\rm UV}$ $\Delta R_{\rm UV}$ $R_{[{\rm OII}]}$ $\Delta R_{[{\rm OII}]}$ $\log{(M_{\rm gas}/M_\odot)}$ $\Delta \log{(M_{\rm gas}/M_\odot)}$

J033210.25-274819.5

 0.6100 PR 150 26 10.29 1.68 -- 5.7 4.1 4.46 0.10 9.80 1.83 9.82 0.33
J033210.76-274234.6 0.4180 CK 550 123 11.44 3.25 5.27 8.5 0.2 4.18 0.08 5.65 0.18 9.89 0.04
J033212.39-274353.6 0.4230 RD 180 22 10.61 1.04 16.18 17.2 0.3 6.27 0.08 8.25 0.94 10.21 0.11
J033213.06-274204.8 0.4220 CK 130 22 10.19 1.69 -- 4.3 2.6 7.29 0.09 18.35 0.86 9.89 0.20
J033214.97-275005.5 0.6680 PR 190 90 10.92 7.01 40.46 47.5 0.7 6.42 0.12 9.19 0.69 10.53 0.08
J033217.62-274257.4 0.6470 CK 250 43 10.38 1.89 16.70 18.6 0.9 3.16 0.11 11.94 2.86 10.24 0.27
J033219.32-274514.0 0.7250 CK 270 29 10.39 2.81 -- 6.4 3.6 3.74 0.12 6.96 1.02 9.78 0.28
J033219.61-274831.0 0.6710 PR 190 33 10.27 3.36 -- 6.7 3.3 2.93 0.11 10.41 1.99 9.89 0.30
J033219.68-275023.6 0.5610 RD 230 33 10.88 5.06 18.61 23.7 0.4 6.75 0.10 12.71 2.31 10.33 0.21
J033220.48-275143.9 0.6790 CK 70 24 10.18 2.15 -- 6.1 3.9 2.54 0.11 15.73 3.19 9.96 0.33
J033224.60-274428.1 0.5380 CK 90 27 10.08 1.72 -- 5.6 3.8 3.88 0.10 8.42 1.55 9.78 0.33
J033225.26-274524.0 0.6660 CK 80 26 10.56 5.05 -- 7.5 2.5 2.92 0.11 10.57 1.74 9.93 0.26
J033226.23-274222.8 0.6679 PR 200 24 10.72 3.17 17.53 20.7 0.8 12.52 0.13 13.84 0.53 10.44 0.04
J033227.07-274404.7 0.7390 CK 110 21 10.26 3.20 -- 6.6 3.4 4.11 0.11 11.18 4.61 9.90 0.44
J033228.48-274826.6 0.6697 CK 130 66 10.63 1.47 34.61 36.1 1.0 1.62 0.11 6.21 1.15 10.28 0.22
J033230.43-275304.0 0.6460 CK 380 29 10.64 1.56 24.67 26.2 1.1 4.88 0.14 9.06 0.59 10.28 0.10
J033230.57-274518.2 0.6810 CK 80 46 11.08 11.24 47.57 58.8 0.7 8.85 0.11 10.28 0.52 10.68 0.05
J033230.78-275455.0 0.6870 RD+ 200 43 10.66 2.92 -- 6.5 3.5 7.61 0.11 7.93 1.71 9.96 0.25
J033231.58-274121.6 0.7047 RD 140 41 10.10 3.22 -- 6.6 3.4 6.28 0.12 12.14 0.08 9.92 0.14
J033232.96-274106.8 0.4690 PR 210 117 10.01 1.45 -- 4.9 3.5 1.24 0.09 6.03 0.15 9.66 0.20
J033233.90-274237.9 0.6190 PR 200 107 10.66 5.69 17.88 23.6 0.6 2.94 0.10 12.92 2.75 10.33 0.24
J033234.04-275009.7 0.7030 RD 160 29 10.09 2.86 -- 6.4 3.6 4.26 0.11 10.52 3.45 9.88 0.40
J033234.12-273953.5 0.6280 CK 110 44 99.99 3.26 25.82 29.1 1.4 3.73 0.12 6.37 1.33 10.25 0.22
J033237.54-274838.9 0.6650 RD 230 71 10.70 7.88 22.26 30.2 0.8 6.53 0.11 11.50 1.65 10.40 0.17
J033238.60-274631.4 0.6220 RD 210 33 10.53 2.13 -- 6.0 3.9 5.91 0.11 11.99 3.47 9.89 0.39
J033239.04-274132.4 0.7330 PR 130 39 10.14 3.60 -- 6.8 3.2 2.84 0.11 10.09 5.14 9.88 0.49
J033239.72-275154.7 0.4160 CK 30 36 10.31 4.19 6.61 10.8 0.3 3.06 0.08 8.87 2.43 10.00 0.29
J033240.04-274418.6 0.5223 CK 470 214 10.77 1.67 15.38 17.1 0.4 1.95 0.09 5.11 0.43 10.00 0.12
J033241.88-274853.9 0.6680 RD+ 120 27 10.27 3.41 -- 6.7 3.3 3.09 0.11 11.29 3.59 9.91 0.39
J033243.62-275232.6 0.6800 PR 60 23 9.86 1.23 -- 5.6 4.4 4.56 0.15 17.04 0.05 9.95 0.20
J033244.20-274733.5 0.7365 CK 170 40 10.62 5.77 61.77 67.5 1.9 1.49 0.11 6.84 2.54 10.50 0.36
J033245.11-274724.0 0.4360 RD 270 44 10.80 1.92 20.77 22.7 0.5 1.63 0.09 4.75 0.56 10.07 0.15
J033248.28-275028.9 0.4462 PR 110 22 10.09 1.98 -- 4.9 2.9 8.77 0.12 14.41 0.94 9.91 0.21
J033249.53-274630.0 0.5230 PR 150 39 10.34 2.74 -- 6.0 3.3 2.98 0.10 7.58 1.72 9.77 0.34
J033250.24-274538.9 0.7318 CK 240 67 10.12 3.06 -- 6.5 3.5 5.51 0.13 6.88 0.26 9.88 0.17
J033250.53-274800.7 0.7370 PR 110 26 10.01 2.10 -- 6.1 4.0 3.83 0.12 6.85 0.18 9.77 0.19

Notes. From left to right: IAU ID, redshift (from Ravikumar et al. 2007), dynamical class (from Yang et al. 2008), rotation velocity and associated uncertainty (from P08), stellar mass $\log{(M_{\rm stellar}/M_\odot)}$ (from P08), SFR$_{\rm UV}$ (in $M_\odot$/yr), SFR$_{\rm IR}$ (in $M_\odot$/yr), total SFR and associated uncertainty $\Delta$SFR (in $M_\odot$/yr), rest-frame UV half-light radius $R_{\rm UV}$ and associated uncertainty $\Delta R_{\rm UV}$ (in kpc), [OII] total radius $R_{[{\rm OII}]}$ and associated uncertainty $\Delta R_{[{\rm OII}]}$ (in kpc), and mass of gas $\log{(M_{\rm gas}/M_\odot)}$ with associated uncertainty $\Delta \log{(M_{\rm stellar}/M_\odot)}$.


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