440 citations · 3.1k across the 28 of their papers we have counts for
13 papers · 1 filter
Constraining the AGN tori at cosmic noon using high-resolution JWST imaging and simultaneous SED fitting
Devang H. Liya, David J. Rosario, Matthaios Charidis
There is evidence for significant evolution in the gaseous and dust properties of galaxies since the era of cosmic noon (). The well known co-evolution of…
Ionized outflows in local luminous AGN: what are the real densities and outflow rates?
R. Davies, D. Baron, T. Shimizu +23
We report on the determination of electron densities, and their impact on the outflow masses and rates, measured in the central few hundred parsecs of 11 local luminous active gala…
The KMOS Survey: rotating compact star forming galaxies and the decomposition of integrated line widths
E. Wisnioski, J. T. Mendel, N. M. Förster Schreiber +23
Using integral field spectroscopy we investigate the kinematic properties of 35 massive centrally-dense and compact star-forming galaxies (, $\log{(Σ_\…
The star formation rates of active galactic nuclei host galaxies
Sara L. Ellison, Hossen Teimoorinia, David J. Rosario +1
Using artificial neural network (ANN) predictions of total infra-red luminosities (LIR), we compare the host galaxy star formation rates (SFRs) of ~21,000 optically selected active…
Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
D. J. Rosario, J. T. Mendel, S. L. Ellison +2
We study a set of 3319 galaxies in the redshift interval 0.04 < z < 0.15 with far-infrared (FIR) coverage from the Herschel Stripe 82 survey (HerS), and emission-line measurements,…
The bulge-disk decomposition of AGN host galaxies
V. A. Bruce, J. S. Dunlop, A. Mortlock +3
We present the results from a study of the morphologies of moderate luminosity X-ray selected AGN host galaxies in comparison to a carefully mass-matched control sample at 0.5 < z…
The infra-red luminosities of ~332,000 SDSS galaxies predicted from artificial neural networks and the Herschel Stripe 82 survey
Sara L. Ellison, Hossein Teimoorinia, David J. Rosario +1
The total infra-red (IR) luminosity (L_IR) can be used as a robust measure of a galaxy's star formation rate (SFR), even in the presence of an active galactic nucleus (AGN), or whe…
Star formation properties of sub-mJy radio sources
M. Bonzini, V. Mainieri, P. Padovani +8
We investigate the star formation properties of ~800 sources detected in one of the deepest radio surveys at 1.4 GHz. Our sample spans a wide redshift range (~0.1 - 4) and about fo…
Decreased Specific Star Formation Rates in AGN Host Galaxies
T. Taro Shimizu, Richard F. Mushotzky, Marcio Melendez +2
We investigate the location of an ultra-hard X-ray selected sample of AGN from the Swift Burst Alert Telescope (BAT) catalog with respect to the main sequence (MS) of star-forming…
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
B. Magnelli, R. J. Ivison, D. Lutz +21
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…
Compton Thick AGN in the XMM-COSMOS survey
G. Lanzuisi, P. Ranalli, I. Georgantopoulos +27
Heavily obscured, Compton Thick (CT, NH>10^24 cm^-2) AGN may represent an important phase in AGN/galaxy co-evolution and are expected to provide a significant contribution to the c…
Large scale clustering measurements with photometric redshifts: comparing the dark matter halos of X-ray AGN, star-forming and passive galaxies at z~1
A. Georgakakis, G. Mountrichas, M. Salvato +11
We combine multiwavelength data in the AEGIS-XD and C-COSMOS surveys to measure the typical dark matter halo mass of X-ray selected AGN [Lx(2-10keV)>1e42 erg/s] in comparison with…
The PEP Survey: Infrared Properties of Radio-Selected AGN
M. Magliocchetti, D. Lutz, D. Rosario +6
By exploiting the VLA-COSMOS and the Herschel-PEP surveys, we investigate the Far Infrared (FIR) properties of radio-selected AGN. To this purpose, from VLA-COSMOS we considered th…