Table 3:

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.

GOODS id	z	morph 1	Mgas			M2/M12	phase3	orbit4	dTmerger5	Tmerger6	Tsfr[Gyr]	(prog)7	(prog)8
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

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  (prog): gas fraction in progenitors. ⁸  (prog): average stellar mass of the progenitors.