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Table 3.

Properties of the individual sources.

Source z log(M*/M) F[O II] F[Ne III] FHβ F[O III] FHα F[S II] SFR 12+log(O/H)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
A2744-YD4
YD4 7.879 8.69 0.17 + 0.18 $ ^{+0.18}_{-0.17} $ 72 ± 3 < 21 36 ± 3 180 ± 4 2.2 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ 8.19 0.13 + 0.09 $ _{-0.13}^{+0.09} $
YD6 7.880 8.40 0.13 + 0.27 $ ^{+0.27}_{-0.13} $ 26 ± 3 < 20 < 17 44 ± 3 < 1.0 8.27 0.20 + 0.16 $ _{-0.20}^{+0.16} $
YD6-[O III]-E 7.881 7.83 0.22 + 0.46 $ ^{+0.46}_{-0.22} $ < 24 < 24 < 14 57 ± 3 < 0.87
YD4-[O III]-W 7.877 7.82 0.48 + 0.41 $ ^{+0.41}_{-0.48} $ < 14 < 15 < 19 46±3 < 1.1
ZD1 7.872 7.58 0.37 + 0.18 $ ^{+0.18}_{-0.37} $ < 13 < 13 < 18 27 ± 3 < 1.1
YD1 7.883 8.58 0.19 + 0.28 $ ^{+0.28}_{-0.19} $ 107 ± 4 < 24 47 ± 3 346 ± 3 2.85 0.18 + 0.18 $ ^{+0.18}_{-0.18} $ 8.11 0.07 + 0.05 $ _{-0.07}^{+0.05} $
YD1-E 7.882 8.44 0.23 + 0.43 $ ^{+0.43}_{-0.23} $ 54 ± 3 < 20 34 ± 2 270 ± 2 2.02 0.13 + 0.13 $ ^{+0.13}_{-0.13} $ 7.98 0.09 + 0.07 $ _{-0.09}^{+0.07} $
s1 7.878 8.01 0.47 + 0.28 $ ^{+0.28}_{-0.47} $ < 24 < 25 18 ± 3 151 ± 3 1.09 0.16 + 0.16 $ ^{+0.16}_{-0.16} $ 7.72 0.20 + 0.20 $ _{-0.20}^{+0.20} $

BDF-3299
a 7.114 7.90 0.13 + 0.25 $ ^{+0.25}_{-0.13} $ 24 ± 2 < 13 36 ± 1 195 ± 3 3.47 0.13 + 0.13 $ ^{+0.13}_{-0.13} $ 7.68 0.09 + 0.13 $ _{-0.09}^{+0.13} $
b 7.114 8.21 0.11 + 0.30 $ ^{+0.30}_{-0.11} $ 28 ± 2 < 11 44 ± 2 285 ± 4 4.2 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ 7.69 0.06 + 0.10 $ _{-0.06}^{+0.10} $
c 7.112 7.62 0.14 + 0.44 $ ^{+0.44}_{-0.14} $ < 13 < 12 15 ± 2 93 ± 4 1.5 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ 7.80 0.38 + 0.15 $ _{-0.38}^{+0.15} $

COSMOS24108
a 6.361 9.29 0.08 + 0.09 $ ^{+0.09}_{-0.08} $ 179 ± 5 48 ± 6 53 ± 5 358 ± 5 219 ± 4 34 ± 4 14.4 1.3 + 1.3 $ ^{+1.3}_{-1.3} $ 8.20 0.06 + 0.05 $ _{-0.06}^{+0.05} $
b 6.358 8.81 0.17 + 0.11 $ ^{+0.11}_{-0.17} $ 150 ± 6 47 ± 6 72 ± 4 470 ± 4 245 ± 3 < 18 9.8 0.3 + 0.3 $ ^{+0.3}_{-0.3} $ 8.11 0.07 + 0.04 $ _{-0.07}^{+0.04} $
c 6.359 8.89 0.06 + 0.10 $ ^{+0.10}_{-0.06} $ 67 ± 5 < 36 28 ± 4 92 ± 4 68 ± 4 < 22 1.74 0.09 + 0.09 $ ^{+0.09}_{-0.09} $ 8.33 0.10 + 0.08 $ _{-0.10}^{+0.08} $
[O III]-Ea 6.362 8.53 0.22 + 0.30 $ ^{+0.30}_{-0.22} $ 62 ± 3 36 ± 3 41 ± 3 296 ± 3 183 ± 3 < 21 14.5 1.3 + 1.3 $ ^{+1.3}_{-1.3} $ 8.01 0.12 + 0.08 $ _{-0.12}^{+0.08} $
[O III]-Eb 6.356 8.40 0.32 + 0.72 $ ^{+0.72}_{-0.32} $ 44 ± 4 < 24 37 ± 3 244 ± 3 113 ± 3 < 22 3.43 0.11 + 0.11 $ ^{+0.11}_{-0.11} $ 7.95 0.17 + 0.14 $ _{-0.17}^{+0.14} $

Notes. (1) Source name. (2) Redshift from [O III]λ5008. (3) Stellar mass from SED fitting with BAGPIPES. (4–9) [O II]λλ3727,30, [Ne III]λ3870, Hβ, [O III]λ5008, Hα, and [S II]λ6718,33 measured fluxes (in units of 10−20 erg s−1 cm−2), (10) SFR (in M yr−1), and (11) gas-phase metallicity from emission line Gaussian fitting. For the sources in the A2744-YD4 system, the reported M* and SFR are corrected for the lensing magnification factor of ∼2 (Morishita et al. 2023; Bergamini et al. 2023); the line fluxes are instead the observed ones. All the properties are obtained from integrated spectra extracted from circular apertures (having radius of 0.15″ for A2744-YD4 and COSMOS24108 and of 0.1″ for BDF-3299) centred on each source. For the line fluxes and SFR, we also report the 3σ upper limits in case of no detection.

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