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Table 6.

Best-fit double Schechter function parameters of the cGSMFs of grouped galaxies for different subsamples, as indicated.

Galaxy sample Halo mass estimator log M α1 α2
( M h 70 2 ) $ (M_{\odot} \, h_{70}^{-2}) $
log ( M dyn M h 70 1 ) 12.5 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 12.5 $ MassA 10.47 ± 0.02 0.14 ± 0.13 –1.25 ± 0.06
log ( M dyn M h 70 1 ) 12.5 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 12.5 $ MassAfunc 10.47 ± 0.03 0.12 ± 0.16 –1.24 ± 0.07
12.5 < log ( M dyn M h 70 1 ) 13 $ 12.5 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13 $ MassA 10.65 ± 0.03 –0.36 ± 0.10 –1.49 ± 0.12
12.5 < log ( M dyn M h 70 1 ) 13 $ 12.5 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13 $ MassAfunc 10.55 ± 0.03 –0.12 ± 0.14 –1.35 ± 0.09
13 < log ( M dyn M h 70 1 ) 13.5 $ 13 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.5 $ MassA 10.78 ± 0.03 –0.40 ± 0.14 –1.34 ± 0.12
13 < log ( M dyn M h 70 1 ) 13.5 $ 13 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.5 $ MassAfunc 10.75 ± 0.02 –0.49 ± 0.09 –1.50 ± 0.14
log ( M dyn M h 70 1 ) > 13.5 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 13.5 $ MassA 11.05 ± 0.01 –0.99 ± 0.04 –0.99 ± 0.08
log ( M dyn M h 70 1 ) > 13.5 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 13.5 $ MassAfunc 11.03 ± 0.01 –0.98 ± 0.06 –0.98 ± 0.09

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