\begin{table}%t3 \caption{\label{tab3}General properties of the 33~distant starbursts, of their progenitors whether they can be assumed to be reproduced by a major merger, as well as merger parameters adopted after the modelling.} \small%\centerline { \begin{tabular}{rrrrr rrrrr rrrr} \hline\hline\noalign{\smallskip} GOODS id & $z$ & morph$_{\rm kin}$$^1$ & Mgas & $M_{\rm stellar}$ & $f_{\rm gas}$ & $M2/M1^2$ & phase$^3$ & orbit$^4$ & dTmerger$^5$ & Tmerger$^6$ & Tsfr[Gyr]& $f_{\rm gas}$ (prog)$^7$ & $M_{\rm stellar}$ (prog)$^8$\\ \hline J033210.25-274819.5 & 0.6087 & 4 & 6.658e+09 & 1.95e+10 & 0.2545 & 0.38 & 1 & 1 & 0.09723 & 0.7134 & 3.398 & 0.2759 & 9.47e+09 \\ J033212.39-274353.6 & 0.4213 & 1 & 1.632e+10 & 4.074e+10 & 0.286 & -- & 5 & -- & -- & -- & 2.366 & -- & -- \\ J033213.06-274204.8 & 0.4215 & 3 & 7.735e+09 & 1.549e+10 & 0.3331 & 0.26 & 2 & 1 & 0.1646 & 0.6334 & 3.614 & 0.3685 & 7.333e+09 \\ J033214.97-275005.5 & 0.6665 & 4 & 3.413e+10 & 8.318e+10 & 0.2909 & 1 & 3 & 2 & 2.399 & 4.532 & 1.752 & 0.9096 & 5.302e+09 \\ J033217.62-274257.4 & 0.6456 & 4 & 1.726e+10 & 2.399e+10 & 0.4184 & 0.7 & 2 & 2 & 0.3429 & 2.062 & 1.29 & 0.4828 & 1.067e+10 \\ J033219.32-274514.0 & 0.7241 & 4 & 5.992e+09 & 2.455e+10 & 0.1962 & 0.55 & 2 & 2 & 0.483 & 1.527 & 3.834 & 0.3214 & 1.036e+10 \\ J033219.61-274831.0 & 0.6699 & 4 & 7.68e+09 & 1.862e+10 & 0.292 & 0.33 & 3 & 3 & 0.6233 & 1.016 & 2.788 & 0.4525 & 7.2e+09 \\ J033219.68-275023.6 & 0.5595 & 1 & 2.136e+10 & 7.586e+10 & 0.2197 & -- & 5 & -- & -- & -- & 3.205 & -- & -- \\ J033220.48-275143.9 & 0.6778 & 4 & 9.086e+09 & 1.514e+10 & 0.3751 & 0.2222 & 2 & 3 & 1.141 & 8.422 & 2.492 & 0.6051 & 4.783e+09 \\ J033224.60-274428.1 & 0.5368 & 4 & 5.961e+09 & 1.202e+10 & 0.3315 & 0.55 & 1 & 2 & 0.07111 & 0.6948 & 2.166 & 0.3455 & 5.886e+09 \\ J033225.26-274524.0 & 0.6647 & 4 & 8.436e+09 & 3.631e+10 & 0.1885 & 0.33 & 3 & 2 & 0.9788 & 1.729 & 4.826 & 0.4773 & 1.169e+10 \\ J033226.23-274222.8 & 0.6671 & 3 & 2.763e+10 & 5.248e+10 & 0.3449 & 0.05 & 5 & -- & 1- & -- & 2.536 & -- & -- \\ J033227.07-274404.7 & 0.7381 & 4 & 7.932e+09 & 1.82e+10 & 0.3036 & 0.33 & 2 & 2 & 0.5716 & 1.01 & 2.758 & 0.432 & 7.421e+09 \\ J033228.48-274826.6 & 0.6685 & 4 & 1.907e+10 & 4.266e+10 & 0.309 & 1 & 3 & 3 & 1.403 & 2.385 & 1.182 & 0.6615 & 1.045e+10 \\ J033230.43-275304.0 & 0.6453 & 4 & 1.91e+10 & 4.365e+10 & 0.3044 & 0.33 & 3 & 3 & 1.373 & 2.425 & 1.664 & 0.6516 & 1.093e+10 \\ J033230.57-274518.2 & 0.6798 & 4 & 4.778e+10 & 1.202e+11 & 0.2844 & 0.33 & 1 & 1 & 0.6125 & 4.582 & 2.044 & 0.4134 & 4.928e+10 \\ J033230.78-275455.0 & 0.6857 & 1 & 9.051e+09 & 4.571e+10 & 0.1653 & -- & 5 & -- & -- & -- & 7.073 & -- & -- \\ J033231.58-274121.6 & 0.7041 & 1 & 8.325e+09 & 1.259e+10 & 0.3981 & -- & 5 & -- & -- & -- & 1.904 & -- & -- \\ J033232.96-274106.8 & 0.4681 & 4 & 4.517e+09 & 1.023e+10 & 0.3062 & 0.33 & 4 & 3 & 0.4033 & 0.5699 & 2.082 & 0.4182 & 4.291e+09 \\ J033233.90-274237.9 & 0.618 & 4 & 2.139e+10 & 4.571e+10 & 0.3188 & 1 & 4 & 4 & 3.06 & 3.66 & 1.939 & 0.801 & 1.061e+10 \\ J033234.04-275009.7 & 0.7016 & 3 & 7.519e+09 & 1.23e+10 & 0.3793 & 1 & 4 & 4 & 0.4955 & 0.5406 & 1.914 & 0.5024 & 4.932e+09 \\ J033234.12-273953.5 & 0.6273 & 4 & 1.763e+10 & 5.012e+10 & 0.2603 & 1 & 3 & 2 & 2.618 & 3.388 & 1.724 & 0.9644 & 1.206e+09 \\ J033237.54-274838.9 & 0.6637 & 1 & 2.492e+10 & 5.012e+10 & 0.3321 & -- & 5 & -- & -- & -- & 1.663 & -- & -- \\ J033238.60-274631.4 & 0.6206 & 1 & 7.71e+09 & 3.388e+10 & 0.1854 & 0.5 & 1 & 5 & 0.0808 & 1.891 & 5.651 & 0.2047 & 1.654e+10 \\ J033239.04-274132.4 & 0.7318 & 4 & 7.641e+09 & 1.38e+10 & 0.3563 & 1 & 4 & 3 & 1.072 & 1.218 & 2.031 & 0.6324 & 3.942e+09 \\ J033239.72-275154.7 & 0.4151 & 4 & 9.879e+09 & 2.042e+10 & 0.3261 & 0.33 & 2 & 1 & 0.3866 & 0.8263 & 1.891 & 0.4101 & 8.936e+09 \\ J033240.04-274418.6 & 0.522 & 4 & 9.991e+09 & 5.888e+10 & 0.1451 & 0.33 & 3 & 4 & 1.381 & 1.878 & 3.453 & 0.5744 & 1.466e+10 \\ J033241.88-274853.9 & 0.667 & 3 & 8.07e+09 & 1.862e+10 & 0.3023 & 1 & 4 & 2 & 1.213 & 1.335 & 2.776 & 0.6409 & 4.792e+09 \\ J033244.20-274733.5 & 0.736 & 4 & 3.155e+10 & 4.169e+10 & 0.4308 & 1 & 3 & 2 & 1.498 & 2.829 & 0.6172 & 0.7408 & 9.49e+09 \\ J033245.11-274724.0 & 0.4346 & 3 & 1.175e+10 & 6.31e+10 & 0.157 & 1 & 4 & 2 & 2.381 & 2.892 & 2.781 & 0.96 & 1.496e+09 \\ J033248.28-275028.9 & 0.4446 & 3 & 8.076e+09 & 1.23e+10 & 0.3963 & 0.33 & 4 & 2 & 0.5944 & 0.7874 & 2.502 & 0.5398 & 4.689e+09 \\ J033249.53-274630.0 & 0.5221 & 4 & 5.923e+09 & 2.188e+10 & 0.2131 & 0.46 & 1 & 1 & 0.05323 & 1.327 & 3.657 & 0.2254 & 1.077e+10 \\ J033250.53-274800.7 & 0.736 & 4 & 5.832e+09 & 1.023e+10 & 0.363 & 0.33 & 3 & 3 & 0.3807 & 0.6207 & 1.692 & 0.4512 & 4.408e+09 \\ \hline \end{tabular}} \medskip Notes: $^1$ morpho-kinematics class following Sect.~2 and Neichel et~al.: 1: rotating VF and spiral morphology; 4: non-relaxed galaxies for which both kinematics and morphologies are discrepant from a rotating disk; 3: other galaxies showing either a rotating VF (and a peculiar morphology) or a complex VF and a spiral morphology. $^2$~$M2/M1$: merger mass ratio for which $M1$ is the mass of the observed galaxy and $M2$ the mass of the interloper. $^3$~Temporal phase: before 1st pass: 1; between 1st and 2nd~pass: 2; near nuclei fusion: 3; disk rebuilding: 4; rotating disk: 5. $^4$~Merger type/orbit: DIR: 1; INC: 2; POL: 3; RET: 4; other/unknown: 5. $^5$~dTmerger: time (in~Gyr) that have been spent by the galaxy in the merger. $^6$~Tmerger: total duration of the merger (in~Gyr). $^7$~$f_{\rm gas}$ (prog): gas fraction in progenitors. $^8$~$M_{\rm stellar}$ (prog): average stellar mass of the progenitors. \end{table}