The 1.4-GHz radio properties of hard X-ray-selected AGN
We have analysed the NRAO Very Large Array Sky Survey and Sydney University Molonglo Sky Survey data at 1.4 GHz and 843 MHz for a well-defined complete sample of hard X-ray AGN observed by INTEGRAL. A large number (70/79) of sources are detected in the radio band, showing a wide range of radio morphologies, from unresolved or slightly resolved cores to extended emission over several hundreds of kpc scales. The radio fluxes have been correlated with the 2-10 keV and 20-100 keV emission,...[Show more]
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Panessa_The_1.4-GHz_radio_properties_2015.pdf||413.36 kB||Adobe PDF||Request a copy|
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