activity
20172022
most citedGalaxy properties of type 1 and 2 X-ray selected AGN and comparison among different classification criteria

49 citations · 140 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202149 cited

Galaxy properties of type 1 and 2 X-ray selected AGN and comparison among different classification criteria

G. Mountrichas, V. Buat, I. Georgantopoulos +4

We present analyses of host galaxy properties of type 1 and type 2 X-ray selected AGNs in the XMM-XXL field, which have available optical spectroscopic classification. We model the…

astro-ph.GA2021

The physical properties of local (U)LIRGs: a comparison with nearby early- and late-type galaxies

E. -D. Paspaliaris, E. M. Xilouris, A. Nersesian +6

In order to pinpoint the place of the (U)LIRGs in the local Universe we examine the properties of a sample of 67 such systems and compare them with those of 268 ETGs and 542 LTGs f…

astro-ph.GA202141 cited

The relation between AGN type and host galaxy properties

V. A. Masoura, G. Mountrichas, I. Georgantopoulos +1

We use 3,213 Active Galactic Nuclei (AGNs) from the -XXL northern field to investigate the relation of AGN type with host galaxy properties. Applying a Bayesian method, w…

astro-ph.GA2020

The survey: XL. Obscuration properties of red AGN in

V. A. Masoura, I. Georgantopoulos, G. Mountrichas +6

The combination of optical and mid-infrared (MIR) photometry has been extensively used to select red active galactic nuclei (AGNs). Our aim is to explore the obscuration properties…

astro-ph.GA2020

A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence

L. P. Grimmett, J. R. Mullaney, E. P. Bernhard +5

Studies investigating the relationship between AGN power and the star formation rates (SFRs) of their host galaxies often rely on averaging techniques -- such as stacking -- to inc…

astro-ph.GA2018

Disentangling the AGN and Star-Formation connection using XMM-Newton

V. A. Masoura, G. Mountrichas, I. Georgantopoulos +3

There is growing evidence supporting the coeval growth of galaxies and their resident SMBH. Most studies also claim a correlation between the activity of the SMBH and the star-form…