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Table B.1

Description of the properties of the star−forming galaxies.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17)
ID_ECDFS RA dec zspec log(M∗/M⊙) SFR E(B−V) log(age/yr) τ Z V errV err 2σNB/fV
deg deg M⊙ yr-1 Gyr Z⊙ 1E+9M⊙
NB3727
23052 53.0090103 −27.7084465 3.263 10.20 13.99 0.15 8.45 0.1 1.0 16.50 ± 2.59 25.39 0.06 0.108 0.234 0.504 9
18320a 53.0135155 −27.7552338 3.213 9.62 6.79 0.00 8.35 0.1 1.0 4.85 ± 0.64 24.43 0.02 −0.034 0.105 0.208 9
21398 53.0145454 −27.7279186 3.132 9.87 9.00 0.06 8.40 0.1 0.2 7.33 ± 1.29 24.75 0.03 0.071 0.132 0.281 10
6839 53.0616188 −27.8462505 3.208 9.81 13.88 0.06 8.30 0.1 0.02 5.77 ± 1.35 24.11 0.02 0.108 0.064 0.155 9
13340 53.0808716 −27.7912197 3.274 9.84 8.47 0.06 8.40 0.1 0.2 8.80 ± 2.16 25.07 0.03 0.124 0.183 0.375 10
26236 53.1133347 −27.6977139 3.168 9.56 6.76 0.03 8.70 0.6 0.02 2.72 ± 0.75 24.89 0.03 −0.054 0.159 0.317 7
5096 53.1165733 −27.8634548 3.287 9.33 0.58 0.00 8.60 0.1 0.02 1.93 ± 0.39 26.31 0.08 −0.312 0.544 1.177 16
697 53.1581573 −27.9257145 3.192 9.15 7.55 0.06 8.40 15.0 0.02 1.14 ± 0.36 25.24 0.02 0.135 0.242 0.437 7
24050 53.1656418 −27.6657372 3.271 9.57 4.57 0.03 8.40 0.1 0.02 2.82 ± 0.94 25.07 0.03 −0.442 0.209 0.377 10
7259 53.1716728 −27.8424492 3.162 9.85 14.98 0.06 8.30 0.1 1.0 6.37 ± 1.76 24.43 0.02 −0.018 0.101 0.207 9
8231 53.2197647 −27.8338223 3.143 10.10 14.02 0.06 8.70 0.3 1.0 9.19 ± 2.04 24.67 0.03 −0.088 0.131 0.259 7
16430 53.1937943 −27.7712898 3.188 9.99 13.67 0.10 8.65 0.3 1.0 9.17 ± 2.41 25.55 0.05 0.031 0.264 0.584 7
17885 53.140419 −27.7592926 3.236 9.80 3.87 0.03 8.50 0.1 1.0 6.52 ± 1.82 25.59 0.04 −0.250 0.283 0.608 10
16526 53.0275917 −27.7702847 3.149 9.86 3.02 0.03 8.55 0.1 1.0 7.54 ± 1.83 25.67 0.05 −0.073 0.322 0.654 10
18454 53.0399857 −27.7540779 3.163 8.82 69.68 0.15 7.00 15.0 0.2 0.08 ± 0.02 25.13 0.04 0.137 0.196 0.396 7
75666 52.9956665 −27.7398472 3.208 10.06 12.97 0.06 8.70 0.3 0.02 − 24.76 0.02 0.005 0.136 0.281 8
59083 53.0544014 −27.9023724 3.232 9.86 9.07 0.00 9.00 3.0 1.0 − 24.61 0.01 0.085 0.110 0.246 7
52315 53.1323662 −27.9521828 3.238 9.34 231.40 0.15 7.00 15.0 1.0 − 24.03 0.02 −0.028 0.086 0.144 4
56382 53.1925201 −27.9246674 3.173 9.53 12.04 0.06 8.60 15.0 0.02 − 25.87 0.05 −0.065 0.436 0.788 7
62873 53.2538567 −27.8633366 3.132 10.40 23.28 0.03 8.90 0.6 0.02 − 23.87 0.01 0.027 0.061 0.124 8
37590 53.019684 −28.045127 3.173 10.14 8.71 0.06 8.50 0.1 0.02 − 25.23 0.03 −0.065 0.213 0.435 12
46323 53.206498 −27.991631 3.153 9.63 17.34 0.03 8.50 2.0 0.2 − 24.62 0.02 0.063 0.125 0.247 7
46783 53.211483 −27.989133 3.192 10.38 29.01 0.06 8.90 1.0 1.0 − 24.93 0.03 0.069 0.178 0.330 7
91256 53.206902 −27.622635 3.278 9.27 18.23 0.10 8.10 2.0 0.2 − 25.51 0.04 −0.073 0.335 0.565 7
82659 53.027626 −27.678058 3.151 8.71 14.09 0.10 7.60 0.3 1.0 − 25.83 0.04 0.454 0.362 0.759 6
79422 52.970582 −27.704338 3.283 8.93 9.84 0.03 8.00 0.6 1.0 − 25.41 0.02 −0.370 0.234 0.515 7
NB387
24919 53.0953941 −27.6875267 3.356 9.51 3.97 0.03 8.40 0.1 0.02 2.48 ± 0.63 25.21 0.04 −0.071 0.050 0.113 10
25151a 53.1433334 −27.690094 3.419 9.79 218.10 0.30 7.50 2.0 0.2 10.30 ± 3.02 24.78 0.03 −0.024 0.033 0.075 5
2584 53.1451225 −27.8903446 3.369 10.28 82.52 0.20 8.50 15.0 1.0 19.80 ± 6.24 24.83 0.02 −0.007 0.035 0.079 7
26325a 53.1785698 −27.7017498 3.412 9.96 19.10 0.06 8.55 0.3 0.2 9.13 ± 1.74 24.57 0.02 −0.028 0.029 0.062 8
18882 53.0257111 −27.7505207 3.403 9.89 6.74 0.03 8.45 0.1 1.0 5.73 ± 1.24 25.28 0.03 0.046 0.052 0.119 9
14354 53.0312309 −27.7852192 3.429 9.90 9.71 0.06 8.40 0.1 0.2 9.12 ± 2.56 25.05 0.04 −0.093 0.051 0.097 10
69899 53.2544556 −27.7927914 3.334 8.46 30.26 0.06 7.00 15.0 0.2 − 25.16 0.02 0.021 0.054 0.107 4
NB388
20417 53.1206131 −27.7365837 3.368 9.92 7.32 0.00 8.75 0.3 1.0 9.08 ± 1.52 24.77 0.02 −0.016 0.019 0.038 8
23842 53.1390076 −27.7152863 3.420 9.85 11.58 0.03 8.35 0.1 1.0 6.47 ± 1.18 24.63 0.02 0.007 0.020 0.034 9
16346 53.1487122 −27.7729473 3.316 9.83 4.30 0.03 8.50 0.1 0.02 0.01 ± 0.00 25.22 0.01 −0.025 0.028 0.058 12
11608 53.2189064 −27.8042641 3.472 9.91 10.63 0.06 9.05 15.0 0.2 7.04 ± 1.44 25.33 0.05 0.016 0.049 0.064 7
13190 53.2286491 −27.7923336 3.327 9.79 3.83 0.03 8.50 0.1 0.02 4.30 ± 2.14 25.28 0.09 −0.027 0.064 0.062 12
15220 53.1332321 −27.7797909 3.469 9.49 5.03 0.03 8.35 0.1 0.2 3.68 ± 0.65 25.38 0.01 0.014 0.032 0.067 9
19760 53.1512985 −27.7429085 3.413 10.25 19.67 0.06 8.70 0.3 1.0 14.00 ± 3.41 24.73 0.02 −0.019 0.018 0.037 8
13734 53.0485344 −27.7886524 3.309 9.27 3.20 0.00 8.60 0.3 0.02 1.49 ± 0.49 25.28 0.04 0.019 0.061 0.061 8
20533 53.1780052 −27.7354355 3.478 9.85 6.57 0.10 8.90 0.6 0.02 5.29 ± 0.97 25.65 0.05 −0.035 0.062 0.087 8
NB396
20583 53.0307884 −27.7348957 3.498 9.43 2.35 0.00 8.45 0.1 0.2 3.76 ± 0.97 25.528 0.049 −0.021 0.160 0.309 12
5764 53.0401802 −27.8563824 3.466 9.64 5.80 0.00 8.80 0.6 0.02 3.02 ± 0.83 24.900 0.015 0.156 0.101 0.173 8
15347 53.0550652 −27.7784977 3.521 9.68 1.32 0.00 8.60 0.1 0.02 4.50 ± 1.25 25.689 0.057 0.095 0.174 0.358 16
4717 53.0617599 −27.8679447 3.473 10.06 20.11 0.06 8.60 0.3 0.02 12.00 ± 4.38 24.436 0.025 0.057 0.067 0.113 8
19613 53.0936394 −27.7440109 3.494 9.96 2.48 0.03 8.60 0.1 0.02 8.54 ± 0.96 25.362 0.039 −0.003 0.129 0.265 16
2324 53.1360855 −27.8937855 3.490 10.02 9.13 0.03 8.45 0.1 1.0 7.62 ± 1.87 24.933 0.023 −0.073 0.086 0.178 9
3325 53.1867943 −27.8814468 3.473 9.87 11.60 0.06 8.90 2.0 0.02 5.27 ± 1.74 25.131 0.025 −0.070 0.104 0.214 7
27939 53.2074356 −27.8796673 3.473 8.44 2.04 0.03 8.00 0.1 0.02 0.33 ± 0.17 26.289 0.097 −0.020 0.313 0.622 7
3768 53.2158508 −27.8768501 3.468 9.74 9.23 0.03 8.60 0.3 1.0 4.48 ± 1.03 25.149 0.038 0.131 0.106 0.218 7
3037 53.2237396 −27.8844109 3.520 9.26 6.18 0.03 8.20 0.1 0.2 1.90 ± 0.49 25.162 0.035 0.059 0.107 0.220 7
3906 53.2173729 −27.8750782 3.466 9.59 4.76 0.03 8.40 0.1 0.02 3.24 ± 0.86 25.114 0.029 0.097 0.104 0.211 10
4022 53.2294273 −27.8742199 3.464 10.27 17.10 0.10 9.00 1.0 0.02 8.83 ± 4.53 25.323 0.052 0.003 0.129 0.255 8
9692 53.0268402 −27.8209667 3.470 9.31 2.52 0.03 8.40 0.1 0.02 2.23 ± 1.15 25.756 0.049 0.338 0.215 0.380 10
7835 53.0394936 −27.8370953 3.456 9.50 305.30 0.35 7.05 15.0 0.2 5.03 ± 1.71 25.489 0.067 −0.201 0.167 0.298 4
20745 53.0459061 −27.7336273 3.498 9.28 2.36 0.03 8.40 0.1 0.02 1.46 ± 0.33 25.857 0.070 0.304 0.205 0.418 10
73615 52.9943237 −27.7592602 3.446 9.63 7.48 0.03 8.60 0.3 0.02 − 25.146 0.025 0.086 0.106 0.217 8
59311 53.0645256 −27.9011326 3.461 9.68 5.78 0.00 8.40 0.1 0.2 − 25.157 0.017 −0.043 0.127 0.219 10
89369 53.1025162 −27.6338024 3.508 8.72 24.27 0.10 7.35 0.1 1.0 − 25.073 0.017 −0.047 0.113 0.203 5
90129 53.1687737 −27.6299114 3.502 10.07 18.85 0.03 8.35 0.1 1.0 − 25.341 0.018 −0.069 0.125 0.260 9
61551 53.2748108 −27.8745422 3.466 10.03 2.96 0.03 8.60 0.1 0.02 − 25.096 0.023 −0.163 0.140 0.207 16
49017 52.993400 −27.972620 3.490 9.78 11.31 0.06 8.70 0.6 0.02 − 25.473 0.029 −0.248 0.141 0.293 7
70198 53.002103 −27.790144 3.470 9.88 28.22 0.10 8.50 1.0 0.02 − 25.113 0.039 0.052 0.120 0.210 7
70236 53.238829 −27.792083 3.489 10.03 17.41 0.03 8.35 0.1 0.2 − 24.207 0.012 0.035 0.068 0.091 9
78739 53.251029 −27.711819 3.475 10.38 15.05 0.03 9.11 1.0 0.2 − 25.073 0.018 −0.171 0.103 0.203 7
83725 53.035204 −27.670960 3.484 9.63 9.05 0.03 8.30 0.1 0.02 − 25.203 0.019 −0.090 0.118 0.229 9

Notes. (1) CANDELS/E-CDFS catalog identification number; (2), (3) right ascension and declination; (4) spectroscopic redshift; (5)−(10) stellar mass, SFR, dust reddening, parametrized by E(B−V), stellar-population age obtained by assuming exponentially declining τ models, τ value in Gyr, and metallicity in solar units. The ratio between τ and stellar-population age is such that the models resemble an instantaneous burst as well as a constant SFR. The SED fit is run fixing the spectroscopic redshift; (11) median mass, taken from the compilation of Santini et al. (2015). It is reported only for sources in CANDELS; (12), (13) V-band AB magnitude taken from CANDELS/GEMS catalogs and its error; (14), (15) ratio between narrow-band and V-band flux densities and its error; (16) ratio between the 2σ background noise of the narrow-band image and the source V-band flux density; (17) intrinsic Lν(1400)/Lν(900) ratio for the age, τ, metallicity in Cols. (8)−(10), and adopting BC03 models.

(a)

Sources already studied in Vanzella et al. (2010a); ID_ECDFS=18320 is Ion2, the source also studied in Vanzella et al. (2015) as a LyC emitter candidate. The sources identified with a 530 million number come from VUDS.

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