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Table 3.

Best fit values and their 1σ uncertainties.

ID zspec log(M/M) (a) t50 AV δ DB Dn4000 f24 μm log Lx log Lx S3 GHz SFR24 μm SFR3GHz
[Gyr] [mag] [mJy] obs. (b) 24 μm [mJy] [M yr−1] [M yr−1]
1 2.841 11.37 0.5 0.2 [−0.7,0] 2.22 ± 0.51 1.47 ± 0.23 < 43.6 0.576 ± 0.03 867 ∼12 930
2 2.557 11.50 0.8 0.1 [−0.4,0] 2.02 ± 0.22 1.34 ± 0.10 (d) < 43.16
3 3.124 11.55 0.4 0.4 [−0.7,0] 2.39 ± 0.19 1.37 ± 0.11 0.041 ± 0.018 < 43.6 43.73 0.011 ± 0.004 < 540 < 307
4 3.230 10.98 0.4 0.1 [−0.7,−0.4] 3.15 ± 0.48 1.21 ± 0.09 0.000 ± 0.024 < 43.6 43.60 0.003 ± 0.003 < 967 < 242
5 2.665 11.34 0.4 0.8 [−0.4] 2.18 ± 0.29 1.39 ± 0.12 0.171 ± 0.017 < 43.6 44.02 0.000 ±0.002 644 < 122
6 2.801 11.36 0.1 1.0 [−0.4] 2.02 ± 0.27 1.34 ± 0.12 0.100 ± 0.021 44.34±0.32 43.91 0.002 ±0.003 508 < 197
7 2.674(c) 11.55 0.7 0.6 [−0.7,0] 2.02 ± 0.35 1.27 ± 0.17 0.111 ± 0.011 44.26 ±0.36 43.89 0.004 ±0.003 419 < 183
8 2.998 11.40 0.7 0.1 [−0.7,−0.4] 2.23 ± 0.2 1.41 ± 0.09 0.000 ± 0.018 < 43.6 43.42 0.002 ±0.002 < 394 < 144
9 2.667 11.53 0.5 [−0.4,0] 2.07 ± 0.41 1.61 ± 0.20 0.032 ± 0.023 < 43.6 43.50 0.005 ±0.003 < 261 < 183
10 2.393 11.33 0.3 1.6 2.25 ± 0.51 1.15 ± 0.15 0.146 ± 0.020 43.73 ± 0.29 43.87 0.005 ± 0.003 289 < 155

Notes. Observed 24 μm and 3 GHz flux densities. Upper limits are given at 3σ.

(a)

Stellar masses are taken from Lustig et al. (2021) and converted to a Salpeter IMF.

(b)

Upper limits for the observed bolometric LX were derived median-stacking all undetected sources.

(c)

Obtained with the addition of NUV-to-NIR broad-band photometry as described in Sect. 4.2.

(d)

ID 2 is absent from the J18 catalogue due to the absence of Ks and VLA 3 GHz priors.

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