2015/07/15 by Т. В. Муфахаров, Mufakharov, T., Yu. V. Sotnikova +5
Physics and Astronomy · Engineering · #Astrophysics and Cosmic Phenomena #Particle Accelerators and Free-Electron Lasers #Gyrotron and Vacuum Electronics Research
paper · pdf · doi:10.48550/arxiv.1507.04283
We have made an estimation of the synchrotron peak frequency (νpeaks) for six very low synchrotron peaked (VLSP) blazars. These objects were selected as VLSP candidates (with the νpeaks ≤ 1013 Hz) from the archival data. We have build spectral energy distribution using quasi-simultaneous observations at the Zeiss-1000 and RATAN-600 telescopes of the Special astrophysical observatory of RAS and made an estimation of the νpeaks. We confirmed classification as a VLSP for two sources ([HB89] 1308+326 and 3C 345), for four other blazars we have calculated νpeaks>1013 Hz.