Table A.1
Summary of stacked properties when stacking as a function of the UV continuum slope.
Redshift range | UV slope range | f160 μm [mJy] | log LUV | log LIR | N |
|
|||||
20.0 ≤ z ≤ 0.5 | −1.4 ≤ β ≤ −1.2 | 1.77±0.19 | 9.61 | 9.98±0.09 | 194 |
20.0 ≤ z ≤ 0.5 | −1.2 ≤ β ≤ −1.0 | 2.73±0.29 | 9.61 | 10.16±0.09 | 121 |
0.5 ≤ z ≤ 1.0 | −1.4 ≤ β ≤ −1.2 | 0.49±0.04 | 9.72 | 10.22±0.07 | 3125 |
0.5 ≤ z ≤ 1.0 | −1.2 ≤ β ≤ −1.0 | 0.82±0.06 | 9.72 | 10.44±0.06 | 2064 |
0.5 ≤ z ≤ 1.0 | −1.0 ≤ β ≤ −0.8 | 1.18±0.08 | 9.73 | 10.60±0.05 | 1244 |
0.5 ≤ z ≤ 1.0 | −0.8 ≤ β ≤ −0.6 | 1.59±0.10 | 9.70 | 10.72±0.05 | 963 |
1.0 ≤ z ≤ 1.5 | −1.4 ≤ β ≤ −1.2 | 0.18±0.02 | 9.86 | 10.28±0.09 | 8136 |
1.0 ≤ z ≤ 1.5 | −1.2 ≤ β ≤ −1.0 | 0.41±0.03 | 9.84 | 10.61±0.06 | 5084 |
1.0 ≤ z ≤ 1.5 | −1.0 ≤ β ≤ −0.8 | 0.65±0.03 | 9.84 | 10.81±0.04 | 4187 |
1.0 ≤ z ≤ 1.5 | −0.8 ≤ β ≤ −0.6 | 0.97±0.05 | 9.81 | 10.98±0.05 | 2634 |
1.0 ≤ z ≤ 1.5 | −0.6 ≤ β ≤ −0.4 | 1.16±0.06 | 9.80 | 11.05±0.04 | 1628 |
1.0 ≤ z ≤ 1.5 | −0.4 ≤ β ≤ −0.2 | 1.54±0.07 | 9.74 | 11.15±0.04 | 1299 |
1.5 ≤ z ≤ 2.0 | −1.2 ≤ β ≤ −1.0 | 0.42±0.03 | 9.98 | 10.92±0.05 | 4359 |
1.5 ≤ z ≤ 2.0 | −1.0 ≤ β ≤ −0.8 | 0.56±0.04 | 9.95 | 11.05±0.06 | 3662 |
1.5 ≤ z ≤ 2.0 | −0.8 ≤ β ≤ −0.6 | 0.77±0.04 | 9.88 | 11.18±0.05 | 2501 |
1.5 ≤ z ≤ 2.0 | −0.6 ≤ β ≤ −0.4 | 1.01±0.06 | 9.83 | 11.31±0.05 | 1691 |
1.5 ≤ z ≤ 2.0 | −0.4 ≤ β ≤ −0.2 | 1.08±0.09 | 9.77 | 11.34±0.07 | 1061 |
1.5 ≤ z ≤ 2.0 | −0.2 ≤ β ≤ −0.0 | 1.11±0.09 | 9.76 | 11.33±0.06 | 825 |
2.0 ≤ z ≤ 2.5 | −1.2 ≤ β ≤ −1.0 | 0.31±0.05 | 10.21 | 11.13±0.15 | 2041 |
2.0 ≤ z ≤ 2.5 | −1.0 ≤ β ≤ −0.8 | 0.62±0.06 | 10.13 | 11.43±0.09 | 1470 |
2.0 ≤ z ≤ 2.5 | −0.8 ≤ β ≤ −0.6 | 0.82±0.09 | 10.07 | 11.53±0.10 | 857 |
2.0 ≤ z ≤ 2.5 | −0.6 ≤ β ≤ −0.4 | 0.73±0.09 | 9.91 | 11.49±0.10 | 776 |
2.0 ≤ z ≤ 2.5 | −0.4 ≤ β ≤ −0.2 | 1.14±0.12 | 9.86 | 11.69±0.08 | 526 |
2.5 ≤ z ≤ 3.0 | −1.2 ≤ β ≤ −1.0 | 0.47±0.07 | 10.40 | 11.56±0.15 | 1001 |
2.5 ≤ z ≤ 3.0 | −1.0 ≤ β ≤ −0.8 | 0.58±0.08 | 10.32 | 11.67±0.13 | 721 |
2.5 ≤ z ≤ 3.0 | −0.8 ≤ β ≤ −0.6 | 0.63±0.13 | 10.22 | 11.69±0.19 | 376 |
Notes. The uncertainties in the rest-frame UV luminosity are related to the normalization of the templates to the observed photometry; they are typically lower than 0.05 dex. The uncertainties in the total IR luminosities are obtained as the difference in the total IR luminosity when considering f160 μm ± Δf160 μm. N indicates the number of galaxies in each bin.
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.