Table 2.
Quantitative comparison of derived parameters with correct and incorrect mirroring.
| Survey | Ngal |  |
 |
 |
|---|---|---|---|---|
| Fornax3D | 12 | 0.832 ± 0.333 | 0.994 ± 0.017 | 0.988 ± 0.153 |
| ATLAS3D | 18 | 1.009 ± 0.039 | 0.992 ± 0.026 | 0.997 ± 0.035 |
| SAMI | 25 | 1.034 ± 0.088 | 1.012 ± 0.019 | 0.999 ± 0.086 |
| Nearly oblate (T ≤ 0.1) | 31 | 1.030 ± 0.193 | 1.003 ± 0.015 | 0.999 ± 0.038 |
| Triaxial (0.1 < T < 0.7) | 25 | 0.997 ± 0.060 | 0.997 ± 0.026 | 1.000 ± 0.021 |
| Nearly prolate (T ≥ 0.7) | 5 | 1.017 ± 0.019 | 0.973 ± 0.044 | 1.002 ± 0.040 |
| All | 61 | 1.010 ± 0.093 | 1.001 ± 0.022 | 0.998 ± 0.032 |
Notes. For each survey, listed in the first column, we list the number of galaxies (Ngal) we considered and the mean ratios between best-fit parameters obtained before and after the bugfix for M/L and for the p and q intrinsic shape parameters. In “all” we also consider the additional galaxies that do not belong to the surveys. Most of these ratios are close to unity, suggesting that very little has changed in the recovered parameters after fixing the mirroring bug.
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