\begin{table}%t1 %\centering \par \caption{Principle properties of the sample of 35 galaxies used in this study, in order of increasing RA (see Sect.~2.5).} \begin{tabular}{cccccccccccccccc}\hline\hline IAU ID & $z$ & D.C. & $V_{\rm flat}$ & $\Delta V_{\rm flat}$ & $\log{(M_{\rm stellar}/M_\odot)}$ & ${\it SFR}_{\rm UV}$ & ${\it SFR}_{\rm IR}$ & ${\it SFR}$ & $\Delta {\it SFR}$ & $R_{\rm UV}$& $\Delta R_{\rm UV}$ & $R_{[{\rm OII}]}$ & $\Delta R_{[{\rm OII}]}$ & $\log{(M_{\rm gas}/M_\odot)}$ & $\Delta \log{(M_{\rm gas}/M_\odot)}$\\\hline \par 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\\\hline \end{tabular} \label{tab} \par \tablefoot{From left to right: IAU ID, redshift (from~\citealt{ravi07}), dynamical class (from~\citealt{yang07}), 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 $\Delta \log{(M_{\rm stellar}/M_\odot)}$.} %\end{table}