Table B.2
Description of the properties of the narrow-band selected Lyα emitters.
(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⊙ | M⊙1E+9 | |||||||||||
|
||||||||||||||||
NB3727 | ||||||||||||||||
|
||||||||||||||||
20433 | 53.065781 | −27.736179 | 3.119 | 9.32 | 3.06 | 0.06 | 9.00 | 15.0 | 0.2 | 2.19 ± 0.52 | 26.11 | 0.05 | 0.052 | 0.466 | 0.975 | 7 |
28279 | 53.229096 | −27.868610 | 3.134 | 8.98 | 0.72 | 0.03 | 8.50 | 0.1 | 0.02 | 0.67 ± 0.30 | 27.16 | 0.18 | 0.522 | 1.240 | 2.563 | 12 |
19293 | 53.053879 | −27.747627 | 3.117 | 10.73 | 61.91 | 0.25 | 9.00 | 2.0 | 1.0 | 45.90 ± 6.67 | 24.92 | 0.05 | −0.106 | 0.161 | 0.327 | 7 |
34808 | 53.180985 | −27.673071 | 3.130 | 8.68 | 0.87 | 0.00 | 8.50 | 0.1 | 0.02 | 0.37 ± 0.08 | 27.37 | 0.21 | −0.790 | 1.691 | 3.131 | 12 |
63466 | 52.978683 | −27.855867 | 3.115 | 8.28 | 20.37 | 0.10 | 7.00 | 15.0 | 1.0 | − | 25.40 | 0.02 | 0.0001 | 0.217 | 0.507 | 4 |
84199 | 53.194806 | −27.666645 | 3.112 | 9.57 | 5.77 | 0.15 | 8.75 | 0.6 | 0.2 | − | 26.73 | 0.05 | −0.150 | 0.962 | 1.730 | 8 |
52172 | 52.971719 | −27.952267 | 3.115 | 9.28 | 2.48 | 0.00 | 9.06 | 15.0 | 2.5 | − | 26.25 | 0.04 | 0.340 | 0.517 | 1.117 | 7 |
71173 | 52.964832 | −27.779763 | 3.108 | 7.21 | 1.41 | 0.00 | 7.10 | 9.0 | 1.0 | – | 26.43 | 0.05 | 0.589 | 0.659 | 1.319 | 5 |
74439 | 52.949147 | −27.750925 | 3.107 | 9.42 | 1.49 | 0.00 | 9.25 | 2.0 | 0.2 | − | 26.63 | 0.05 | −0.897 | 0.782 | 1.574 | 7 |
− (a) | 53.078858 | −27.644502 | 3.122 | − | − | − | − | − | − | − | 26.88 | 0.07 | −1.082 | 0.950 | 1.991 | − |
46913 | 52.959872 | −27.986139 | 3.123 | 7.83 | 2.45 | 0.00 | 7.50 | 2.0 | 1.0 | − | 26.50 | 0.04 | 0.460 | 0.724 | 1.396 | 6 |
− a | 53.236134 | −27.830346 | 3.102 | − | − | − | − | − | − | − | 26.82 | 0.06 | −0.747 | 0.994 | 1.874 | − |
− a | 53.278931 | −27.707732 | 3.111 | − | − | − | − | − | − | − | 26.91 | 0.07 | 0.270 | 0.967 | 2.044 | − |
− a | 52.999277 | −27.829559 | 3.120 | − | − | − | − | − | − | − | 26.07 | 0.04 | −0.475 | 0.457 | 0.940 | − |
− a | 53.367375 | −28.055773 | 3.122 | − | − | − | − | − | − | − | 27.35 | 0.07 | −0.326 | 1.553 | 3.070 | − |
− a | 53.043862 | −27.988235 | 3.122 | − | − | − | − | − | − | − | 27.02 | 0.05 | −0.100 | 1.236 | 2.269 | − |
− a | 53.131038 | −27.726939 | 3.133 | − | − | − | − | − | − | − | 26.99 | 0.11 | −0.985 | 1.111 | 2.196 | − |
75954 | 53.348875 | −27.735881 | 3.114 | 8.50 | 1.38 | 0.00 | 8.50 | 15.0 | 0.2 | − | 27.05 | 0.09 | −1.311 | 1.121 | 2.322 | 7 |
− a | 53.351875 | −27.742758 | 3.113 | − | − | − | − | − | − | − | 27.61 | 0.13 | −2.904 | 1.895 | 3.903 | − |
Notes. (1) Identification number from CANDELS/E-CDFS catalog; (2), (3) right ascension and declination in degrees; (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 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.
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