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Table 7.

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
NFOF > 4 ( M h 70 2 ) $ (M_{\odot} \, h_{70}^{-2}) $
log ( M lum M h 70 1 ) 13.75 $ \log \left(\frac{M_{\mathrm{lum}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.75 $ LumB 10.74 ± 0.04 –0.33 ± 0.22 –1.23 ± 0.11
log ( M dyn M h 70 1 ) 13.75 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.75 $ MassA 10.88 ± 0.03 –0.67 ± 0.12 –1.40 ± 0.18
log ( M lum M h 70 1 ) 13.75 $ \log \left(\frac{M_{\mathrm{lum}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.75 $ LumBfunc 10.88 ± 0.03 –0.70 ± 0.12 –1.48 ± 0.20
log ( M dyn M h 70 1 ) 13.75 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 13.75 $ MassAfunc 10.87 ± 0.03 –0.69 ± 0.11 –1.47 ± 0.19
13.75 < log ( M dyn M h 70 1 ) 14.25 $ 13.75 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 14.25 $ LumB 11.12 ± 0.02 –1.01 ± 0.07 –1.01 ± 0.10
13.75 < log ( M dyn M h 70 1 ) 14.25 $ 13.75 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 14.25 $ MassA 11.10 ± 0.02 –1.04 ± 0.17 –1.04 ± 0.06
13.75 < log ( M dyn M h 70 1 ) 14.25 $ 13.75 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 14.25 $ LumBfunc 11.10 ± 0.02 –1.00 ± 0.02 –1.00 ± 0.04
13.75 < log ( M dyn M h 70 1 ) 14.25 $ 13.75 < \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) \leq 14.25 $ MassAfunc 11.08 ± 0.02 –1.01 ± 0.18 –1.01 ± 0.06
log ( M dyn M h 70 1 ) > 14.25 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 14.25 $ LumB 11.07 ± 0.03 –1.02 ± 0.09 –1.02 ± 0.08
log ( M dyn M h 70 1 ) > 14.25 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 14.25 $ MassA 11.11 ± 0.02 –1.08 ± 0.07 –1.08 ± 0.06
log ( M dyn M h 70 1 ) > 14.25 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 14.25 $ LumBfunc 11.06 ± 0.02 –1.04 ± 0.13 –1.04 ± 0.05
log ( M dyn M h 70 1 ) > 14.25 $ \log \left(\frac{M_{\mathrm{dyn}}}{M_{\odot}\,h^{-1}_{70}}\right) > 14.25 $ MassAfunc 11.13 ± 0.02 –1.10 ± 0.02 –1.10 ± 0.05

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