EMU is a wide-field radio continuum survey planned for the new Australian Square
Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep …

We present an updated mid-infrared (MIR) versus X-ray correlation for the local active
galactic nuclei (AGN) population based on the high angular resolution 12 and 18μm …

We carry out a comprehensive Bayesian correlation analysis between hot halos and direct
masses of supermassive black holes (SMBHs), by retrieving the X-ray plasma properties …

We combine Chandra and XMM–Newton X-ray data from our previous papers with new X-
ray observations and with Spitzer mid-infrared (mid-IR) data in order to study the nature of …

Kiloparsec-scale binary active galactic nuclei (AGNs) signal active supermassive black hole
(SMBH) pairs in merging galaxies. Despite their significance, unambiguously confirmed …

We present two-dimensional gaseous kinematics of the inner 1.1× 1.6 kpc2 of the Seyfert 2
galaxy NGC 2110, from optical spectra (5600–7000 Å) obtained with the Gemini Multi Object …

We present a two-dimensional mapping of the gas flux distributions, as well as of the gas
and stellar kinematics in the inner 220 pc of the Seyfert galaxy NGC 2110, using K-band …

We have studied the X-ray emission within the inner∼ 150 pc radius of NGC 4151 by
constructing high spatial resolution emission line images of blended O vii, O viii, and Ne ix …

We present a detailed analysis of the XMM–Newton Reflection Grating Spectrometer (RGS)
high-resolution X-ray spectra of the Seyfert 2 galaxy, Mrk 573. This analysis is …

Abstract We investigate the 1.4-GHz radio properties of 92 nearby (z< 0.05) ultra-hard X-ray
selected active galactic nuclei (AGNs) from the Swift Burst Alert Telescope (BAT) sample …