All Tables

Table 1: GPS sources. Columns 1 through 13 provide source name, optical identification (G: galaxy, Q: quasar, EF: empty field), optical magnitude ("V'',"R'' are the bands in the optical, "r'' band-defined by Stanghellini et al. 1993), redshift (those with * are a photometric estimate by Heckman et al. 1994), linear scale factor pc/mas [ $H_{0}=100~ h~ \rm km~s^{-1}~ Mpc^{-1}$ and q₀=0.5 have been assumed], maximum VLBI angular size fromPapers I, II or this observation, maximum VLBI linear size, 5 GHz total flux density measured at Effelsberg, low frequency spectral index, high frequency spectral index, turnover frequency, peak flux density and references for the spectral information (Refs. 1, de Vries et al. 1997; 2, Stanghellini et al. 1998; 3, Dallacasa et al. 2000; 4, O'Dea et al. 1996; 5, Spoelstra et al. 1985).
Table 2: Integrated properties of the sources from the WSRT data, values of EVPA are likely to be meaningless for objects with $m \leq$ 0.4%.
Table 3: Parameters of the components in the VLBI images at 5 GHz. The columns give: (1) source name and possible classification (CSOc: Compact Symmetric Object candidate, cj: core-jet); (2) total image intensity measured with IMEAN at 5 GHz; (3) component identification labled to Xiang et al. (2002, 2005); (4), (5) peak (per beam) and integral intensity of component at 5 GHz measured with JMFIT; (6),(7) major/minor axes (with error $\leq$ 10%) and position angle of component at 5 GHz measured with JMFIT; (8), (9) distance and position angle relative to the first component; (10) brightness temperature of component; (11) integrated fractional polarization in source.