Unveiling the Nature of Unidentified γ-Ray Sources. VI. γ-Ray Blazar Candidates in the WISH Survey and their Radio Properties

According to the Fermi Large Area Telescope Second Source Catalog (2FGL), about one-third of the γ -ray sources listed have no assigned counterparts at lower energies.Many statistical methods have been developed to find proper counterparts for these sources. We explore the sky area covered at low radio frequency by the Westerbork in the Southern Hemisphere (WISH) survey to search for blazar-like associations among the unidentified γ -ray sources (UGSs) listed in the 2FGL. Searching the WISH and NRAO Very Large Array Sky Survey radio surveys within the positional uncertainty regions of the 2FGL UGSs, we select as γ -ray blazar candidates the radio sources characterized by flat radio spectra between 352 MHz and 1400 MHz. We propose new γ -ray blazar associations for eight UGSs and we also discuss their spectral properties at low radio frequencies. We compare the radio flux density distribution of the low radio frequency γ -ray blazar candidates with that of γ -ray blazars associated with other methods. We find significant differences between these distributions. Finally, we discuss the results of this association method and its possible applicability to other regions of the sky and future radio surveys.