  We report the first detection at 4.7 and 8.2 GHz with the RATAN-600 radio
telescope of the source PSO J047.4478+27.2992, which has been announced as a
blazar at z=6.1. The average flux density is $12\pm3$ and $8\pm4$ mJy at 4.7
and 8.2 GHz respectively, and an upper limit is estimated as 3 mJy at 11.2 GHz.
The light curve at 4.7 GHz, obtained on a time-scale of four months, exhibits
moderate variability of the source (fractional variability
$F_{var}=0.28\pm0.02$). The new RATAN-600 measurements extend previous
literature data to higher frequencies, indicating a single power-law radio
spectrum with $\alpha_{0.147-8.2}$=$-0.51\pm0.1$. The monochromatic radio
luminosity at 4.7 GHz $P_{\nu} \sim 2 \times 10^{27}$ W Hz$^{-1}$ is consistent
with values for high-redshift quasars at $z\geq 3$.
