Discovery of a suspected giant radio galaxy with the KAT-7 array
arXiv:1511.08330 · doi:10.1093/mnras/stv2693
Abstract
We detect a new suspected giant radio galaxy (GRG) discovered by KAT-7. The GRG core is identified with the WISE source J013313.50-130330.5, an extragalactic source based on its infrared colors and consistent with a misaligned AGN-type spectrum at . The multi- spectral energy distribution (SED) of the object associated to the GRG core shows a synchrotron peak at Hz consistent with the SED of a radio galaxy blazar-like core. The angular size of the lobes are for the NW lobe and for the SE lobe, corresponding to projected linear distances of kpc and kpc, respectively. The best-fit parameters for the SED of the GRG core and the value of jet boosting parameter , indicate that the GRG jet has maximum inclination deg with respect to the line of sight, a value obtained for , while the minimum value of is not constrained due to the degeneracy existing with the value of Lorentz factor . Given the photometric redshift , this GRG shows a core luminosity of W Hz, and a luminosity W Hz for the NW lobe and W Hz for the SE lobe, consistent with the typical GRG luminosities. The radio lobes show a fractional linear polarization consistent with typical values found in other GRG lobes.
7 pages, 6 figures, 2 tables, accepted for publication in MNRAS
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