Table C.7
Quality of the fundamental plane as a distance indicator using our selected sample of 94 922 elliptical galaxies, but with the direct-fit coefficients of Bernardi et al. (2003c) or Hyde & Bernardi (2009), respectively (the coefficients are listed in Table 1 of this paper).
| Filters | s ε |  [%] |
|
|
||
| Bernardi et al. (2003c) | ||
| g | 0.1056 | 16.8 |
| r | 0.1054 | 17.9 |
| i | 0.1028 | 16.8 |
| z | 0.1134 | 16.0 |
|
|
||
| Hyde & Bernardi (2009) | ||
| g | 0.1063 | 18.8 |
| r | 0.1042 | 17.5 |
| i | 0.1031 | 17.4 |
| z | 0.1087 | 18.6 |
Notes. We found that our best-fit coefficients (see Table 5) are better by a few percent than those of our esteemed colleagues.
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