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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(BV) log(age/yr) τ Z V errV err 2σNB/fV
deg deg M yr-1 Gyr Z M1E+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(BV), 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.

(a)

Sources detected in GEMS, but without counterpart in the photometric CDF-S catalog.

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