Abstract:
Measurements of the flux densities of the extended components of seven giant radio galaxies
obtained using the RATAN-600 radio telescope at wavelengths of 6.25 and 13 cm are presented. The
spectra of components of these radio galaxies are constructed using these new RATAN-600 data together
with data from theWENSS, NVSS, and GB6 surveys. The spectral indices in the studied frequency range
are calculated, and the need for detailed estimates of the integrated contribution of such objects to the
background emission is demonstrated.
