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The 1.4-GHz radio properties of hard X-ray-selected AGN

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Date

2015-02-21

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Abstract

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, revealing significant correlations with slopes consistent with those expected for radiatively efficient accreting systems. The high-energy emission coming from the inner accretion regions correlates with the radio emission averaged over hundreds of kpc scales (i.e. thousands of years).

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Keywords

Active-galaxies, Galaxies, Seyfert-radio continuum

Citation

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https://dspace-test.anu.edu.au/handle/1885/733751447

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DevOps Pure Testing

Source

Monthly Notices of the Royal Astronomical Society

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Article

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DOI

10.1093/mnras/stu2455

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