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Table 4.

Best-fit double Schechter function parameters of the GSMFs of star-forming and passive galaxies, corresponding to blue and red populations in other studies, as indicated.

Sample log M α1 α2
( M h 70 2 $ M_{\odot}\,h_{70}^{-2} $)
Global – Peng et al. (2010) 10.67 ± 0.01 −0.52 ± 0.04 −1.56 ± 0.12
Global – Weigel et al. (2016) 10.79 ± 0.01 −0.79 ± 0.04 −1.69 ± 0.10
Global – this work 10.84 ± 0.01 −0.72 ± 0.03 −1.58 ± 0.03

Blue – Peng et al. (2010) 10.63 ± 0.01 ... −1.40 ± 0.01
Blue – Weigel et al. (2016) 10.60 ± 0.01 ... −1.21 ± 0.01
Star-forming – this work 10.48 ± 0.02 −0.08 ± 0.09 −1.44 ± 0.02

Red – Peng et al. (2010) 10.68 ± 0.01 −0.39 ± 0.03 (−1.56)
Red – Weigel et al. (2016) 10.77 ± 0.01 −0.45 ± 0.02 −2.46 ± 0.33
Passive – this work 10.83 ± 0.01 −0.48 ± 0.02 −2.30 ± 0.22

Blue D1 – Peng et al. (2010) 10.60 ± 0.01 ... −1.39 ± 0.02
Star-forming ungrouped – this work 10.38 ± 0.02 0.07 ± 0.11 −1.50 ± 0.02

Blue D4 – Peng et al. (2010) 10.64 ± 0.02 ... −1.41 ± 0.04
Star-forming grouped – this work 10.52 ± 0.02 0.11 ± 0.13 −1.32 ± 0.03

Red D1 – Peng et al. (2010) 10.61 ± 0.01 −0.36 ± 0.05 (−1.56)
Passive ungrouped – this work 10.58 ± 0.01 −0.08 ± 0.04 −2.27 ± 0.15

Red D4 – Peng et al. (2010) 10.76 ± 0.02 −0.55 ± 0.06 (−1.56)
Passive grouped – this work 10.92 ± 0.01 −0.50 ± 0.03 −2.00 ± 0.28

Notes. Ellipses in the α1 column denote that a single Schechter function was used. Values of α2 shown in parentheses without uncertainties were not fitted but just fixed to the global value adopted in the corresponding study.

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