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Table 1
Comparison between parameters of HOD for satellite galaxies obtained by Yang et al. (2008) and by our method.
Yang et al. (2008) | Background subtraction | |||
M lim | M 0 | α | M 0 | α |
|
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−16.0 | −−−−−− | −−−−−− | 11.9 ± 0.6 | 0.97 ± 0.03 |
−16.5 | −−−−−− | −−−−−− | 12.0 ± 0.5 | 0.98 ± 0.03 |
−17.0 | −−−−−− | −−−−−− | 12.1 ± 0.5 | 0.99 ± 0.03 |
−17.5 | −−−−−− | −−−−−− | 12.2 ± 0.5 | 1.00 ± 0.03 |
−18.0 | 12.48 ± 0.04 | 1.01 ± 0.06 | 12.3 ± 0.6 | 1.01 ± 0.03 |
−18.5 | 12.62 ± 0.02 | 1.05 ± 0.04 | 12.4 ± 0.6 | 1.03 ± 0.03 |
−19.0 | 12.77 ± 0.02 | 1.06 ± 0.03 | 12.6 ± 0.6 | 1.04 ± 0.03 |
−19.5 | 12.93 ± 0.01 | 1.07 ± 0.02 | 12.8 ± 0.6 | 1.05 ± 0.03 |
−20.0 | 13.15 ± 0.01 | 1.09 ± 0.02 | 13.0 ± 0.7 | 1.06 ± 0.05 |
−20.5 | 13.44 ± 0.01 | 1.10 ± 0.02 | 13.3 ± 0.7 | 1.11 ± 0.05 |
−21.0 | 13.82 ± 0.01 | 1.13 ± 0.02 | 13.7 ± 0.7 | 1.13 ± 0.05 |
−21.5 | 14.34 ± 0.01 | 1.33 ± 0.07 | 14.2 ± 0.7 | 1.33 ± 0.05 |
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