Table 1.
Origins of data used in this paper.
| Source | Number of objects | Selection | Redshift | Note |
|---|---|---|---|---|
| Bouwens et al. (2016) | 3 | UV | 5 ≲ z ≲ 10 | * ALMA 6 upper limits |
| * S/NHST > 1.5 | ||||
| * LBGs with > 5 data points in UV-optical only | ||||
| Capak et al. (2015) and Faisst et al. (2017) | 9 (HZ1-HZ4 and HZ6-HZ10) | UV | z ∼ 5.6 | * [CII]158 μm for all Hi-z LBGs |
| * ALMA 7 detections: HZ4, HZ6 (3) HZ9 and HZ10 (5) | ||||
| * ALMA 7 upper limits for the others | ||||
| * HZ5 detected in Chandra and not included in the sample | ||||
| * 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 and WMH5) | UV | z ∼ 6.1 | * ALMA 6 detections |
| * [CII]158 μm measurement | ||||
| Aravena et al. (2016) | 2 (ID27, ID31) | UV | z ∼ 7.5 | * ALMA 6 detections |
| * [CII]158 μm measurement | ||||
| Hashimoto et al. (2018) | 1 (MACSJD1149) | UV | z = 9.1 | * ALMA 7 upper limit |
| * [OIII]88 μm measurement | ||||
| Rémy-Ruyer et al. (2015) | 31 | DGS and Z < 0.1 Z⊙ | z ∼ 0 | * GALEX FUV and NUV data from NED |
| * B and R data from NED | ||||
| * IR data (including Herschel) from Rémy-Ruyer et al. (2013) and Rémy-Ruyer et al. (2015) | ||||
Notes. The Hi-z LBG sample contains 18 objects, while the Low-zZ sample contains 31 objects for which the final fits are adequate, i.e. 
. 9 Hi-z LBGs are detected in ALMA in Band 6 or Band 7, they provide 15 detected measurements, but only 11 measurements with S/Nsubmm > 3 are used to build the IR template.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.