All Tables

Table 1: All Fornax cluster members detected in the FCOS, ordered by magnitude. The object codes are "FCOS x-xxx'' for FCOS-1 (Mieske et al. 2002) and "FCOS x-xxxx'' for FCOS-2 (this paper). Errors in V and (V-I) are between 0.04 and 0.05 mag, as judged from the artificial star experiments described in Sect. 4.2.1. ^*For all objects FCOS 0-2xxx, V and (V-I) are derived indirectly from the C-R photometry of Dirsch et al. (2003), using V=R+0.5 mag and (V-I)=(C-R)-0.5 mag (see text for further details). ^** $v_{\rm rad}$ is the mean of the values measured in FCOS-1 and FCOS-2 (see text for further details).
Table 2: Table showing the mean velocities $\overline {v}$ and velocity dispersions $\sigma _v$ of all, only bright (V<20 mag) and only faint (V>20 mag) Fornax members. Samples considered are: the entire FCOS-sample (FCOS-1 and FCOS-2); the FCOS-sample corrected for the systematic velocity differences between FCOS-1 and FCOS-2 (see Sects. 3.1 and 4.1); and the shift corrected FCOS-sample + additional Fornax members from Dirsch et al. (2004) + the 2 UCDs not observed in the FCOS, taken from Karick et al. (2003). The column "Dif. Conf.'' gives the confidence limit in percent for the hypothesis of the bright and faint value being different, derived with a t-test for the means and with an F-test for the dispersions.