Table B.1
Schechter parameters (M∗, α, φ∗) and total luminosity density LD for the rest-frame FUV- and NUV-band galaxy luminosity function for the VVDS Deep+Ultra-Deep sample with the cosmology (Ωm, ΩΛ, h) = (0.3, 0.7, 0.7).
| FUV | NUV | ||||||||
| Redshift rangea |
|
α | φ∗ | lg(LDuc)b |
|
α | φ∗ | lg(LDuc)b | |
| (AB mag) | (10-3 Mpc-3) | W/Hz/Mpc3 | (AB mag) | (10-3 Mpc-3) | W/Hz/Mpc3 | ||||
|
|
|||||||||
| Free Schechter parameters | |||||||||
| 0.05 < z ≤ 0.2 |
|
|
|
18.86 |
|
|
|
18.90 |
|
| • | 0.2 < z ≤ 0.4 |
|
|
|
18.87 |
|
|
|
18.97 |
| • | 0.4 < z ≤ 0.6 |
|
|
|
18.85 |
|
|
|
18.99 |
| • | 0.6 < z ≤ 0.8 |
|
|
|
18.93 |
|
|
|
19.12 |
| • | 0.8 < z ≤ 1.0 |
|
|
|
19.04 |
|
|
|
19.27 |
| • | 1.0 < z ≤ 1.2 |
|
|
|
19.12 |
|
|
|
19.30 |
| • | 1.2 < z ≤ 1.7 |
|
|
|
19.13 |
|
|
|
19.28 |
| 1.7 < z ≤ 2.5 |
|
|
|
19.70 |
|
|
|
19.56 |
|
| 2.5 < z ≤ 3.5 |
|
|
|
19.17 |
|
|
|
19.37 |
|
| 3.5 < z ≤ 4.5 | − | − | − | − | − | − | − | − | |
|
|
|||||||||
| M∗ constrainedc, α and φ∗ free | |||||||||
| • | 0.05 < z ≤ 0.2 | −18.12 |
|
|
18.76 |
||||
|
|
|||||||||
| α constrainedd, M∗ and φ∗ free | |||||||||
| • | 1.7 < z ≤ 2.5 |
|
−1.30 |
|
19.46 |
||||
| • | 2.5 < z ≤ 3.5 |
|
−1.50 |
|
19.40 |
||||
| • | 3.5 < z ≤ 4.5 |
|
−1.73 |
|
19.10 |
||||
| 1.7 < z ≤ 2.5 |
|
−1.10 |
|
19.41 |
|||||
| 2.5 < z ≤ 3.5 |
|
−1.10 |
|
19.24 |
|||||
| 3.5 < z ≤ 4.5 |
|
−1.10 |
|
18.73 |
|||||
| 1.7 < z ≤ 2.5 |
|
−1.73 |
|
19.79 |
|||||
| 2.5 < z ≤ 3.5 |
|
−1.73 |
|
19.62 |
|||||
Notes.
The entries labelled with a filled dot are the chosen Schechter parameters taken for the rest-frame FUV LF used throughout the paper, and reported in Table 1.
The quoted errors are those induced by the STY LF fit; see Table 1 for errors including also other sources of uncertainty.
M∗ is set at z ≤ 0.2 assuming the local rest-frame FUV value determined by Wyder et al. (2005).
α is set with different values at z > 1.7. First, following an evolution with redshift as described in Sect. 3.2 (α = −1.3, −1.5, −1.73 at 1.7 < z ≤ 2.5, 2.5 < z ≤ 3.5, 3.5 < z ≤ 4.5, respectively); secondly, set as two likely extreme non-evolving values (α = −1.1 and α = −1.73). We remind that α = −1.1 corresponds to what we find at 1.2 < z ≤ 1.7 (where we can still determine α with a reasonable error), and α = −1.73 is the value found by Bouwens et al. (2007) at z = 3.8. Contrarily to the rest-frame FUV LF, we were not interested in setting any Schechter parameters for the rest-frame NUV LF.
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