Data di Pubblicazione:
2014
Abstract:
A well known property of the γ -ray sources detected by Cos-B in the 1970s, by the Compton Gamma-Ray
Observatory in the 1990s, and recently by the Fermi observations is the presence of radio counterparts, particularly
for those associated with extragalactic objects. This observational evidence is the basis of the radio–γ -ray connection
established for the class of active galactic nuclei known as blazars. In particular, the main spectral property of
the radio counterparts associated with γ -ray blazars is that they show a flat spectrum in the GHz frequency
range. Our recent analysis dedicated to search blazar-like candidates as potential counterparts for the unidentified
γ -ray sources allowed us to extend the radio–γ -ray connection in the MHz regime. We also showed that blazars
below 1 GHz maintain flat radio spectra. Thus, on the basis of these new results, we assembled a low-frequency
radio catalog of flat-spectrum sources built by combining the radio observations of the Westerbork Northern Sky
Survey and of the Westerbork in the southern hemisphere catalog with those of the NRAO Very Large Array
Sky survey (NVSS). This could be used in the future to search for new, unknown blazar-like counterparts of
γ -ray sources. First, we found NVSS counterparts of Westerbork Synthesis Radio Telescope radio sources, and
then we selected flat-spectrum radio sources according to a new spectral criterion, specifically defined for radio
observations performed below 1 GHz. We also described the main properties of the catalog listing 28,358 radio
sources and their logN–logS distributions. Finally, a comparison with the Green Bank 6 cm radio source catalog was
performed to investigate the spectral shape of the low-frequency flat-spectrum radio sources at higher frequencies.
Tipologia CRIS:
03A-Articolo su Rivista
Keywords:
galaxies: active , quasars: general , radiation mechanisms: non-thermal , surveys
Elenco autori:
F. Massaro;M. Giroletti;R. D'Abrusco;N. Masetti;A. Paggi;Philip S. Cowperthwaite;G. Tosti;S. Funk
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