activity
20122019
most citedEvidence that the AGN dominates the radio emission in z ~ 1 radio-quiet quasars

66 citations · 280 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2019

Accretion and star formation in 'radio-quiet' quasars

Sarah V. White, Matt J. Jarvis, Eleni Kalfountzou +4

Radio observations allow us to identify a wide range of active galactic nuclei (AGN), which play a significant role in the evolution of galaxies. Amongst AGN at low radio-luminosit…

astro-ph.HE2019★ 5 cited

CIELO-RGS: a catalogue of soft X-ray ionized emission lines

Junjie Mao, J. S. Kaastra, M. Guainazzi +9

High-resolution X-ray spectroscopy has advanced our understanding of the hot Universe by revealing physical properties like kinematics, temperature, and abundances of the astrophys…

astro-ph.HE2018★ 25 cited

A high velocity component to the complex absorption in IRAS 13349+2438

M. L. Parker, G. A. Matzeu, M. Guainazzi +4

We present an analysis of XMM-Newton spectra of the low-redshift quasar IRAS 13349+2438. The RGS spectrum shows a large number of absorption lines from two zones of warm absorption…

astro-ph.GA2017★ 28 cited

SDSS J1056+5516: A Triple AGN or an SMBH Recoil Candidate?

Eleni Kalfountzou, M. Santos Lleo, M. Trichas

We report the discovery of a kiloparsec-scale triple supermassive black hole system at : SDSS J1056+5516, discovered by our systematic search for binary quasars. The syste…

astro-ph.GA2017★ 25 cited

Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

E. Kalfountzou, J. A. Stevens, M. J. Jarvis +6

Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the…

astro-ph.GA2017★ 66 cited

Evidence that the AGN dominates the radio emission in z ~ 1 radio-quiet quasars

Sarah V. White, Matt J. Jarvis, Eleni Kalfountzou +4

In order to understand the role of radio-quiet quasars (RQQs) in galaxy evolution, we must determine the relative levels of accretion and star-formation activity within these objec…