0922+005 [Q, z = 1.72]
The radio spectrum of this quasar turned out to be flat between 5 and 0.4 GHz
and therefore the turnover cannot be clearly determined. The radio emission is
resolved at S band in PA~45^deg^. At X band again the source is just resolved in
PA~30^deg^. This source was not detected at 2.3 MHz in a single baseline
experiment by Morabito et al. (1986). Our VLBI images account for ~55% and 65%
of the total flux density at S and X bands respectively.