Open Access
Table 1.
Fitted formulas.
| Formula | RMS | Nout | a | b | c | d | Uncertainties |
|---|---|---|---|---|---|---|---|
| aMg + b | 0.1703 | 14 | −0.499 | 0.427 | – | – | ±0.003, 0.051 |
| aMr + b | 0.1271 | 14 | −0.476 | 0.597 | – | – | ±0.002, 0.037 |
| aMz + b | 0.1788 | 22 | −0.415 | 1.668 | – | – | ±0.002, 0.047 |
| aMg + bMr + c | 0.0972 | 24 | 0.673 | −1.108 | 0.996 | – | ±0.019, 0.018, 0.031 |
| aMg + bMz + c | 0.1505 | 20 | −0.276 | −0.191 | 0.877 | – | ±0.010, 0.008, 0.050 |
| aMr + bMz + c | 0.1236 | 17 | −0.416 | −0.054 | 0.703 | – | ±0.007, 0.006, 0.039 |
| aMg + bMr + cMz + d | 0.0957 | 25 | 0.657 | −1.062 | −0.028 | 1.056 | ±0.019, 0.019, 0.004, 0.032 |
Notes. Parameters, RMS values, and the number of discarded outlying galaxies (Nout) of different fitting formulas for calculating log(M*[M⊙]) using galaxy total magnitudes in different bands.
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