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Table B.1

Description of the properties of the starforming 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(BV) 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(BV), 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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