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Table C.1.

Measurements and physical parameters of our galaxies from the VVDS-Ultra Deep sample.

ID α δ Redshift zflag MgUV, d MgUV, f M⋆ SFR E(B − V)s Ageonset Agepass tf D4000 Cat
910265695 36.8548 −4.3850 0.5116 3 1.034 1.330 8.820 −0.021 0.350 0.719 0.619 8.17 1.36 S
910378108 36.7234 −4.1341 0.5163 4 1.100 1.141 8.283 −0.304 0.150 0.453 0.353 8.40 1.34 C
910274705 36.8722 −4.3647 0.5249 3 1.071 1.154 8.891 0.070 0.300 0.806 0.706 7.99 1.32 S
910359082 36.8471 −4.1759 0.5556 3 1.092 1.134 9.014 −0.076 0.200 1.610 1.210 6.97 1.40 S
910360899 36.6654 −4.1718 0.559 2 1.699 1.723 9.446 −1.295 0.100 1.610 1.410 6.94 1.96 S
910342467 36.6655 −4.2113 0.5633 3 1.448 1.163 8.819 −0.373 0.100 0.453 0.353 8.07 1.46 S
910367269 36.7979 −4.1581 0.588 4 1.216 1.196 8.832 −0.747 0.050 0.509 0.409 7.85 1.57 S
910193981 36.8630 −4.5428 0.6125 3 1.270 1.211 10.243 −0.197 0.150 1.280 0.880 6.91 1.85 C
910202695 36.8607 −4.5225 0.6326 3 1.316 1.148 9.280 −0.920 0.050 2.300 1.900 5.76 1.65 C
910245811 36.8194 −4.4287 0.7833 2 1.155 1.076 9.118 −0.232 0.200 0.453 0.353 6.73 1.10 C
910195196 36.5937 −4.5407 0.7926 24 1.383 1.779 10.910 −1.741 0.000 2.300 2.100 4.84 1.99 S
910260329 36.6642 −4.3965 0.8612 3 1.517 1.217 10.179 −0.558 0.150 2.600 2.200 4.19 1.86 S
910296534 36.7009 −4.3160 0.8622 2 2.030 2.146 9.631 −1.076 0.100 0.806 0.706 5.98 1.86 S
910160900 36.8599 −4.6170 1.0259 3 1.711 1.621 10.308 −3.974 0.000 1.610 1.510 4.44 1.92 S
910197254 36.4191 −4.5349 1.0389 3 1.347 1.290 10.381 −1.625 0.050 1.140 1.040 4.86 1.91 S
910267731 36.4422 −4.3802 1.0537 3 1.601 1.554 10.771 −1.998 0.000 2.300 2.100 3.64 1.99 S
910215192 36.4405 −4.4960 1.0562 3 1.382 1.630 10.633 −3.633 0.000 1.610 1.510 4.32 1.92 S
910191001 36.6485 −4.5484 1.118 3 1.411 1.850 10.785 −5.407 0.000 2.300 2.200 3.40 1.98 S
910157260 36.8575 −4.6239 1.1256 2 1.230 1.208 10.381 −0.728 0.100 1.800 1.600 3.87 1.47 S
910174325 36.8734 −4.5860 1.2703 3 1.415 1.632 10.724 −4.472 0.000 2.600 2.400 2.57 2.04 S
910216226 36.5994 −4.4930 1.2851 3 1.376 1.207 10.513 −0.494 0.100 1.610 1.410 3.51 1.39 S
910191575 36.7054 −4.5464 1.2968 3 1.316 1.244 10.489 −0.601 0.000 1.610 1.410 3.48 1.86 S
910189008 36.4484 −4.5526 1.3273 2 1.423 1.748 10.828 −1.840 0.050 1.430 1.330 3.56 1.43 S
910332932 36.7953 −4.2322 1.361 3 1.201 1.293 9.708 1.728 0.350 0.181 −0.019 4.71 1.16 S
910251093 36.8421 −4.4163 1.3868 3 1.869 1.546 10.803 −1.899 0.000 1.280 1.180 3.54 2.09 S
910334635 36.7042 −4.2286 1.3912 1 1.392 1.505 11.160 −1.538 0.000 1.430 1.330 3.38 1.41 S
910159830 36.8157 −4.6189 1.424 3 1.532 1.551 10.993 −1.083 0.050 1.280 1.180 3.43 1.91 S
910261703 36.7752 −4.3948 1.4331 3 1.384 1.472 11.000 −0.407 0.050 1.020 0.920 3.67 1.89 S
910262816 36.8060 −4.3916 1.4807 3 1.234 1.159 10.674 −0.094 0.000 0.905 0.805 3.66 1.81 S
910200844 36.8252 −4.5270 1.5017 2 1.500 1.389 10.481 −1.425 0.000 1.140 1.040 3.37 1.86 S
910191908 36.8375 −4.5460 1.5067 2 1.272 1.132 11.165 0.098 0.100 1.140 0.940 3.36 1.88 S
910374671 36.8381 −4.1414 1.54 2 1.436 1.150 10.868 −1.803 0.000 1.280 1.180 3.13 1.89 S
910293115 36.6150 −4.3242 1.895 2 1.355 1.247 9.912 1.322 0.150 0.719 0.619 2.94 1.31 S
910294781 36.6049 −4.3203 2.0578 1 1.181 1.247 9.815 1.553 0.150 0.360 0.260 3.02 1.17 C
910182978 36.6228 −4.5676 2.1432 4 1.244 1.169 10.016 2.008 0.200 0.181 0.081 3.06 1.15 C
910259852 36.7312 −4.3975 2.1527 1 1.355 1.204 10.557 2.001 0.400 0.286 0.186 2.94 1.32 C
910195919 36.6249 −4.5374 2.2461 3 1.209 1.209 −99.9 −99.9 −99.9 0.0 −99.9 −99.9 −99.9 C

Notes. For each galaxy we provide identification, coordinates (α, δ), redshift, and redshift flag (zflag; see Le Fèvre et al. 2015 for more details); measurements of MgUV from data and best spectral fit; stellar masses (M⋆) and SFR (both given in log10 scales); the dust extinction (E(B − V)s); Ageonset and Agepassive (both in Gyr); and D4000 indexes and formation epoch (in cosmic time and in gigayear since the Big Bang). We also give the sample ID (S: secure, C: candidate). Some galaxies appear with a value of −99.9 for the physical parameters. This means that they could not be fitted owing to a lack of photometric points.

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