Speaker
Francesca Panessa
(National Institute for Astrophysics - INAF)
Description
We have characterized the radio emission in a complete sample
of AGN observed at hard X-rays by INTEGRAL and Swift. The majority of the sources have been detected at 1.4 GHz, displaying a variety of radio fluxes and morphologies,
from strong jet sources to very faint weak unresolved components.
The observed emission is then compared to the X-ray and hard X-ray emission,
to check for a possible relationship between the disk-corona
and the jet/outflow emission.
Author
Francesca Panessa
(National Institute for Astrophysics - INAF)
