Table E.1.
Logarithmic SMF values for the total, SF, and Q galaxy samples.
| Bin | log(M★/M⊙) | log10(Φtot) [dex−1 Mpc−3] | log10(ΦSF) [dex−1 Mpc−3] | log10(ΦQ) [dex−1 Mpc−3] |
|---|---|---|---|---|
| 1 | 9.13 | −2.0570 ± 0.0069 | −2.140 ± 0.019 | −2.93 ± 0.18 |
| 2 | 9.37 | −2.1101 ± 0.0049 | −2.256 ± 0.036 | −2.682 ± 0.077 |
| 3 | 9.62 | −2.2255 ± 0.0039 | −2.474 ± 0.036 | −2.595 ± 0.056 |
| 4 | 9.87 | −2.3089 ± 0.0029 | −2.526 ± 0.041 | −2.562 ± 0.036 |
| 5 | 10.12 | −2.3410 ± 0.0018 | −2.674 ± 0.045 | −2.520 ± 0.036 |
| 6 | 10.37 | −2.4112 ± 0.0018 | −2.830 ± 0.067 | −2.565 ± 0.027 |
| 7 | 10.62 | −2.4841 ± 0.0019 | −3.149 ± 0.092 | −2.592 ± 0.025 |
| 8 | 10.87 | −2.7122 ± 0.0027 | −3.70 ± 0.12 | −2.757 ± 0.014 |
| 9 | 11.12 | −3.1249 ± 0.0045 | −4.50 ± 0.17 | −3.1439 ± 0.0073 |
| 10 | 11.37 | −3.7352 ± 0.0090 | −5.31 ± 0.34 | −3.7471 ± 0.0092 |
Notes. These are the measured binned SMFs shown in Figs. 8 and D.1. Units are dex−1 Mpc−3. The quoted uncertainties are propagated logarithmic errors. Bins with log M★ < Mlim(z = 0.2) are not complete over the full redshift range; however, the SMF is computed using the redshift-dependent completeness function Mlim(z) derived with the method of Pozzetti et al. (2010), shown in Fig. 6.
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