Open Access
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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