All Tables

Table 1: Observation log and properties of observed objects. V₀ is from Evstigneeva et al. (2006) and (V-I)₀ from Mieske et al. (2006) (except (V-I)₀ for FCC303 which is from Karick et al. 2003). Both, V₀ and (V-I)₀ are corrected for foreground dust extinction (Schlegel et al. 1998). The [Fe/H] values are from Mieske et al. (2006).
Table 2: Observation log and properties of standard stars that were used as velocity dispersion templates. They are ordered by their increasing metallicity. Most of the properties were taken from the SIMBAD database, see: http://simbad.u-strsbg.fr/Simbad
Table 3: Wavelength regions for direct fitting of velocity dispersions and prominent lines therein. The values are given in the restframe.
Table 4: Results of velocity dispersion measurements in all direct fitting regions (same identification numbers as in Table 3). On the left, the results from the blue part of the spectrum are shown, and on the right the ones from the red part. The identification numbers of the three best fitting templates are given in brackets below each $\sigma _v$ value. The S/N are those for the combined spectra at the given wavelength.
Table 5: Average values for radial velocity and velocity dispersion measurements: (1) mean of all fits; (2) as (1), but with 2-sigma clipping; (3) mean excluding Na and Ca region and combined region. The values in bold face are those used for further analyses. The velocity dispersion of UCD1 was derived by Drinkwater et al. (2003) from Keck spectroscopy.
Table 6: Mass modelling results for different light profile representations. The modelled projected half-light radius $r_{\rm h,p}$ , central velocity dispersion $\sigma _0$ , global velocity dispersion $\sigma$ , mass and mass-to-light ratio in the V-band are given. The adopted surface brightness profile parameters are taken from Evstigneeva et al. (2006). Radii ( $R_{\rm b}$ , $R_{\rm e}$ , $R_{\rm c}$ and $R_{\rm t}$ ) are in pc; $\mu _{\rm0,King}$ and $\mu _{e,\rm Sers.}$ are in mag arcsec^-2 in the V band. In the last rows the results for the virial mass estimator are given. The effective radius $R_{\rm eff}$ was taken from Table 10 of Evstigneeva et al. (2006), the global velocity dispersion from the generalized King models and King + Sersic models in two-component fits case. Also the ellipticies ( $\epsilon = 1-b/a$ ) from Evstigneeva et al. are shown for reference. The values in bold face were adopted for further analyses.