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Table 6

Galaxy properties.

ID Δv (km s-1) E(B − V)β E(B − V)β − α E(B − V)SED log (M/M) 12+log (O/H)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

BX1 2.6 ± 2.5 2.5 ± 0.6 0.8 ± 0.1 125.1 ± 108.1 0.12 ± 0.02 ≤0.54 0.32 9.25 ≥8.2
BX10 ≥0.6 0.49 ± 0.17 749.0 ± 205.8 0.12 ± 0.02 0.32
BX16 1.7 ± 0.6 − 897.8 ± 272.3 0.35 ± 0.02 ≤ 0.01 0.10
BX4 0.35 ≥8.4
BX7 0.35 ≤8.5
BX14 4.0 ± 3.2 0.3 ± 0.5 0.35 ≤8.6
LBG11 0.37 ± 0.14 344.5 ± 107.0 0.07 ± 0.14 ≥ 0.1 ≥ 9.95 ≤9.0
LAE27 0.08 ± 0.02 167.8 ± 105.3 ≤ 0.1
z3LAE2 0.11 ± 0.03 221.8 ± 90.0 0.32
z2LAE2 0.09
DB8 0.47
DB12 4.4 ± 3.3 0.42 ± 0.20 0.26
DB22

Notes. Column 1: names of the sources as presented in Table 3. Column 2−4: Hα/Hβ, Lyα/Hα, and Lyα/[OIII]5007 line flux ratios. Column 5: velocity offsets calculated using Eq. (5). Column 6−8: dust-reddening estimations, obtained from fitting the rest-frame UV slope (E(B − V)β), the Balmer decrement (E(B − V)β − α) in the 2nd column, and from SED fitting (E(B − V)SED). If continuum is too low to estimate β slope we do not report E(B − V)β. BX16 spectrum provides F(Hα)/F(Hβ) = 1.7 ± 0.6, i.e. F(Hα)/F(Hβ) < 2.9 at 2σ, which is consistent with no reddening (E(B − V)β − α ≤ 0.01). Column 9: stellar masses in unit of solar metallicity (M/M), inferred from the SED fit. Column 10: metallicity values taken from the final column of Table 5.

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