Table 2.
Properties and fit results of our characteristic spectra.
| ID | Name | R/B–R | Radius (pixels) | χ 2/N | SN1/SN2 | Norm.factor (102) | Vr (km s−1) | σ(km s−1) |
|---|---|---|---|---|---|---|---|---|
| 1 | Nucleus A | 21.1/1.06 | 2 | 0.68 | 18/22 | 3.09 | 3621.6 | 1.0 |
| 2 | Region B | 21.3/0.65 | 3 | 0.81 | 22/29 | 5.95 | 3622.3 | 0 |
| 3 | Region C | 21.5/0.83 | 2 | 0.71 | 19/18 | 2.52 | 3644.2 | 18 |
| 4 | R15minusABC | R15-ABC | 0.39 | 23/32 | 95.9 | 3623.2 | 15 | |
| 5 | R30–R15 | – | 15–30 | 2.52 | 18/104 | 179 | 3618.9 | 7 |
| 6 | R40 | – | 40 | 2.27 | 22/115 | 340 | 3622.2 | 10 |
Notes. Name, R-magnitude colour B−R, extraction radius, χ 2/N. SN1 is the S/N that STARLIGHT finds from comparison with the model spectra, and SN2 is the S/N that corresponds to the flux uncertainty provided by the STAT part of the MUSE cube. The normalisation factor is used for calculating absolute fluxes. The last columns are the heliocentric radial velocity and the velocity dispersion. Magnitude and colour are from Richtler et al. (2015). We give the kinematical data without interpretation.
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