The polar diagram of synchrotron radiation from the developed steady n
arrow jet in the radial magnetic field of the active core of an extrag
alactic object is calculated. Calculations were done for the normalize
d frequency and two spectral indices of emitting particles: gamma = 1.
4 and 2.5. The frequency dependence found is not typical for a known r
elativistic jet model. The maximum number of detected sources consiste
nt with model gamma = 2.5 is shown to be reached at frequency 18 GHz.
The fraction of such sources directed to the observer and emitting at
this frequency is evaluated to be of 0.09.