All Tables

• Table 1: Radio emission data of the sources in the three epochs of the observations (a = 22 Aug. 1998; b = 10 Sep. 1998; c = 21 Sep. 1998). Column [1], IAU name; Col. [2] optical id.; Col. [3] redshift (values in parentheses are photometric redshifts, using the GPS galaxy Hubble diagram); Cols. [4]-[7] flux density of the arc second core and any additional radio emission at 1.36 and 1.66 GHz (values in parentheses indicate that in our judgment, the radio emission likely comes from an unrelated object). Flux density errors for compact strong components are dominated by the calibration uncertainties estimated around 3, while for extended weak components the flux density errors are dominated by the limits of the self-cal/imaging process in the presence of a strong source nearby, and the flux densities given can be considered only rough estimates. *  It accounts for the region South of the arcsecond core only.