The best-fitting relation (log(MS) = β × log(M200) + α) on the stellar mass and halo mass plane in observations and SAMs.
| Subsamples . | β . | α . |
|---|---|---|
| S-I: | ||
| Obs | 1.05 ± 0.3 | −3.01 ± 3.9 |
| G11 | 0.45 ± 0.02 | 5.08 ± 0.23 |
| B06 | 0.43 ± 0.03 | 5.18 ± 0.38 |
| DLB07 | 0.36 ± 0.02 | 6.26 ± 0.21 |
| S-II: | ||
| Obs | 0.38 ± 0.24 | 5.85 ± 3.26 |
| G11 | 0.46 ± 0.04 | 4.88 ± 0.56 |
| B06 | 0.47 ± 0.07 | 4.56 ± 0.92 |
| DLB07 | 0.39 ± 0.04 | 5.87 ± 0.52 |
| S-III: | ||
| Obs | 0.48 ± 0.21 | 4.56 ± 2.89 |
| G11 | 0.5 ± 0.02 | 4.3 ± 0.27 |
| B06 | 0.33 ± 0.03 | 6.4 ± 0.43 |
| DLB07 | 0.43 ± 0.02 | 5.35 ± 0.26 |
| S-IV: | ||
| Obs | 0.36 ± 0.23 | 6.06 ± 3.12 |
| G11 | 0.49 ± 0.03 | 4.36 ± 0.42 |
| B06 | 0.29 ± 0.05 | 6.87 ± 0.65 |
| DLB07 | 0.4 ± 0.03 | 5.63 ± 0.37 |
| S-V: | ||
| Obs | 0.71 ± 0.37 | 1.2 ± 5.11 |
| G11 | 0.48 ± 0.05 | 4.5 ± 0.72 |
| B06 | 0.43 ± 0.08 | 4.94 ± 1.15 |
| DLB07 | 0.43 ± 0.05 | 5.2 ± 0.66 |
| Subsamples . | β . | α . |
|---|---|---|
| S-I: | ||
| Obs | 1.05 ± 0.3 | −3.01 ± 3.9 |
| G11 | 0.45 ± 0.02 | 5.08 ± 0.23 |
| B06 | 0.43 ± 0.03 | 5.18 ± 0.38 |
| DLB07 | 0.36 ± 0.02 | 6.26 ± 0.21 |
| S-II: | ||
| Obs | 0.38 ± 0.24 | 5.85 ± 3.26 |
| G11 | 0.46 ± 0.04 | 4.88 ± 0.56 |
| B06 | 0.47 ± 0.07 | 4.56 ± 0.92 |
| DLB07 | 0.39 ± 0.04 | 5.87 ± 0.52 |
| S-III: | ||
| Obs | 0.48 ± 0.21 | 4.56 ± 2.89 |
| G11 | 0.5 ± 0.02 | 4.3 ± 0.27 |
| B06 | 0.33 ± 0.03 | 6.4 ± 0.43 |
| DLB07 | 0.43 ± 0.02 | 5.35 ± 0.26 |
| S-IV: | ||
| Obs | 0.36 ± 0.23 | 6.06 ± 3.12 |
| G11 | 0.49 ± 0.03 | 4.36 ± 0.42 |
| B06 | 0.29 ± 0.05 | 6.87 ± 0.65 |
| DLB07 | 0.4 ± 0.03 | 5.63 ± 0.37 |
| S-V: | ||
| Obs | 0.71 ± 0.37 | 1.2 ± 5.11 |
| G11 | 0.48 ± 0.05 | 4.5 ± 0.72 |
| B06 | 0.43 ± 0.08 | 4.94 ± 1.15 |
| DLB07 | 0.43 ± 0.05 | 5.2 ± 0.66 |
The best-fitting relation (log(MS) = β × log(M200) + α) on the stellar mass and halo mass plane in observations and SAMs.
| Subsamples . | β . | α . |
|---|---|---|
| S-I: | ||
| Obs | 1.05 ± 0.3 | −3.01 ± 3.9 |
| G11 | 0.45 ± 0.02 | 5.08 ± 0.23 |
| B06 | 0.43 ± 0.03 | 5.18 ± 0.38 |
| DLB07 | 0.36 ± 0.02 | 6.26 ± 0.21 |
| S-II: | ||
| Obs | 0.38 ± 0.24 | 5.85 ± 3.26 |
| G11 | 0.46 ± 0.04 | 4.88 ± 0.56 |
| B06 | 0.47 ± 0.07 | 4.56 ± 0.92 |
| DLB07 | 0.39 ± 0.04 | 5.87 ± 0.52 |
| S-III: | ||
| Obs | 0.48 ± 0.21 | 4.56 ± 2.89 |
| G11 | 0.5 ± 0.02 | 4.3 ± 0.27 |
| B06 | 0.33 ± 0.03 | 6.4 ± 0.43 |
| DLB07 | 0.43 ± 0.02 | 5.35 ± 0.26 |
| S-IV: | ||
| Obs | 0.36 ± 0.23 | 6.06 ± 3.12 |
| G11 | 0.49 ± 0.03 | 4.36 ± 0.42 |
| B06 | 0.29 ± 0.05 | 6.87 ± 0.65 |
| DLB07 | 0.4 ± 0.03 | 5.63 ± 0.37 |
| S-V: | ||
| Obs | 0.71 ± 0.37 | 1.2 ± 5.11 |
| G11 | 0.48 ± 0.05 | 4.5 ± 0.72 |
| B06 | 0.43 ± 0.08 | 4.94 ± 1.15 |
| DLB07 | 0.43 ± 0.05 | 5.2 ± 0.66 |
| Subsamples . | β . | α . |
|---|---|---|
| S-I: | ||
| Obs | 1.05 ± 0.3 | −3.01 ± 3.9 |
| G11 | 0.45 ± 0.02 | 5.08 ± 0.23 |
| B06 | 0.43 ± 0.03 | 5.18 ± 0.38 |
| DLB07 | 0.36 ± 0.02 | 6.26 ± 0.21 |
| S-II: | ||
| Obs | 0.38 ± 0.24 | 5.85 ± 3.26 |
| G11 | 0.46 ± 0.04 | 4.88 ± 0.56 |
| B06 | 0.47 ± 0.07 | 4.56 ± 0.92 |
| DLB07 | 0.39 ± 0.04 | 5.87 ± 0.52 |
| S-III: | ||
| Obs | 0.48 ± 0.21 | 4.56 ± 2.89 |
| G11 | 0.5 ± 0.02 | 4.3 ± 0.27 |
| B06 | 0.33 ± 0.03 | 6.4 ± 0.43 |
| DLB07 | 0.43 ± 0.02 | 5.35 ± 0.26 |
| S-IV: | ||
| Obs | 0.36 ± 0.23 | 6.06 ± 3.12 |
| G11 | 0.49 ± 0.03 | 4.36 ± 0.42 |
| B06 | 0.29 ± 0.05 | 6.87 ± 0.65 |
| DLB07 | 0.4 ± 0.03 | 5.63 ± 0.37 |
| S-V: | ||
| Obs | 0.71 ± 0.37 | 1.2 ± 5.11 |
| G11 | 0.48 ± 0.05 | 4.5 ± 0.72 |
| B06 | 0.43 ± 0.08 | 4.94 ± 1.15 |
| DLB07 | 0.43 ± 0.05 | 5.2 ± 0.66 |
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