Table 2.
Results of the power law fitting of the MSR.
| Samples | ⟨z⟩ | log a | b | n | log M*/M⊙ |
|---|---|---|---|---|---|
| range | |||||
| ET vol1 | 0.33 | −3.41 ± 0.63 | 0.37 ± 0.07 | 37 | 6.03–10.80 |
| ET vol2 | 0.77 | −3.53 ± 0.56 | 0.38 ± 0.06 | 68 | 8.48–11.12 |
| ET vol3 | 1.11 | −5.42 ± 3.31 | 0.56 ± 0.32 | 17 | 9.97–10.92 |
| LT vol1 | 0.34 | −1.87 ± 0.13 | 0.24 ± 0.02 | 749 | 5.42–10.78 |
| LT vol2 | 0.79 | −1.21 ± 0.13 | 0.18 ± 0.01 | 964 | 7.40–11.91 |
| LT vol3 | 1.39 | −1.41 ± 0.18 | 0.20 ± 0.02 | 1160 | 7.77–11.06 |
| ET all | 0.66 | −3.44 ± 0.32 | 0.38 ± 0.03 | 122 | 6.03–11.12 |
| LT all | 0.88 | −1.74 ± 0.06 | 0.23 ± 0.01 | 2873 | 5.42–11.91 |
Notes. Redshift bins are defined as follows: vol1: z < 0.5, vol2: 0.5 ≤ z < 1, and vol3: 1 ≤ z < 2. Median redshift for each volume and type is given in Col. 2. For each bin we fit a single power law according to Eq. (2), with the number of galaxies and stellar mass range indicated in the two last columns. These are shown in Fig. 11. The last two rows give the results of fit using all the sources in ET and LT samples – both are shown in Fig. 12.
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