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Table 1.
Best-fit values for the inclination bias in the M*, r1/2, and n, using Eq. (4).
| a | b | c | ||
|---|---|---|---|---|
| log(M*[M⊙]) | 0.13 ± 0.14 | 0.26 ± 0.42 | 10.28 ± 0.15 | |
| SDSS | r1/2 (kpc) | 3.78 ± 0.16 | 3.35 ± 0.25 | 4.47 ± 0.049 |
| n | −0.49 ± 0.029 | 2.94 ± 0.32 | 3.43 ± 0.034 | |
| log(M*[M⊙]) | 2.84 ± 120 | 82.2 ± 143 | 9.86 ± 0.015 | |
| GAMA | r1/2 (kpc) | 3.79 ± 0.15 | 5.16 ± 0.37 | 3.72 ± 0.042 |
| n | −0.35 ± 0.047 | 2.73 ± 0.82 | 1.00 ± 0.024 | |
| log(M*[M⊙]) | 0.25 ± 0.067 | 4.56 ± 2.09 | 9.97 ± 0.018 | |
| COSMOS | r1/2 (kpc) | 8.07 ± 0.36 | 3.75 ± 0.31 | 3.71 ± 0.12 |
| n | −0.58 ± 0.057 | 3.54 ± 0.67 | 0.92 ± 0.02 | |
Notes. GAMA seems to have an inclination independent mass log(M*[M⊙]), causing large uncertainties in the inclination dependent fitting parameters a and b.
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