Table 1.
Galaxy sample properties.
| Galaxy | MUSE | K-Phot. | log Mdyn, e | tS/N | Ngal | σ★ |
|---|---|---|---|---|---|---|
| NGC 3512 | AMUSING | UHS | 9.64 | 50 | 2 | 81.3 |
| NGC 1285 | AMUSING | VHS | 10.15 | 60 | 1 | 93.4 |
| NGC 5248 | TIMER | VHS | 10.24 | 100 | 3 | 91.7 |
| NGC 3521 | MAD | VIKING | 10.29 | 260 | 1 | 126.0 |
| IC 2560 | MAD | VHS | 10.39 | 100 | 5 | 117.1 |
| NGC 1566 | PHANGS | VHS | 10.38 | 200 | 13 | 241.9 |
| NGC 7364 | AMUSING | UKIDSS | 10.50 | 60 | 1 | 147.1 |
| NGC 0863 | AMUSING | UKIDSS | 10.78 | 80 | 2 | 312.5 |
Notes. Identifiers, parent MUSE surveys, K-band photometry sources (VISTA: VHS/VIKING; UKIRT: UKIDSS/UHS), logarithmic dynamical masses at the effective radius obtained with DYNAMITE, target continuum signal-to-noise ratios for Voronoi binning, number of galaxies in the host group (environment information provided by Tempel et al. 2016), and light-weighed average stellar velocity dispersion within the bulge.
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