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Table 1.

Origins of the data used in this paper.

Source Number of Selection Redshift Notes
objects
Le Fèvre et al. (2020), Faisst et al. (2020a), Bethermin et al. (2020) 118 SFG z ∼ 4.5 – 20 ALMA-7 detections with S/N > 3
z ∼ 5.5 – 78 ALMA-7 upper limits
– 18 ALMA-7 not selected (not enough data)
– S/NUV-optical-NIR > 2.5.
– SFG with > 5 data points in UV-optical only
– [CII]158 μm measurements for 64% of the sample

Capak et al. (2015); Faisst et al. (2017) 4 (HZ4, HZ6, UV z ∼ 5.6 – [CII]158 μm for all Hi-z LBGs
HZ9, HZ10
– ALMA-7 detections: HZ4, HZ6 (3) HZ9 & HZ10 (5)
– ALMA-7 upper limits for the others
– HZ5 detected in Chandra and not included in thesample
– Additional data from Pavesi et al. (2016)

Scoville et al. (2016) 1 (566428) UV z = 5.89 – ALMA-6 detection
– [CII]158 μm measurement

Willott et al. (2015) 2 (CLM1 & WMH5) UV z ∼ 6.1 – ALMA-6 detections
– [CII]158 μm measurement

Notes. The final sample used in this paper contains 105 objects: 27 with ALMA detections and 78 with ALMA upper limits. The other objects were discarded from the sample because they do not have enough data in the UV-optical-near-IR range to perform a safe SED fitting.

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