\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}