activity
20122017
most citedFar-infrared Fine-Structure Line Diagnostics of Ultraluminous Infrared Galaxies

175 citations · 479 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2017★ 17 cited

Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster

Kathryn A. Harris, Victor P. Debattista, Fabio Governato +9

Using a cosmological -body simulation, we investigate the origin and distribution of stars in the intracluster light (ICL) of a Fornax-like cluster. In a dark matter only simula…

astro-ph.GA2016★ 48 cited

Extreme star formation events in quasar hosts over

Lura K. Pitchford, Evanthia Hatziminaoglou, Anna Feltre +7

We explore the relationship between active galactic nuclei and star formation in a sample of 513 optically luminous type 1 quasars up to redshifts of 4 hosting extremely high…

astro-ph.GA2016★ 27 cited

The Geometry of the Infrared and X-ray Obscurer in a Dusty Hyperluminous Quasar

Duncan Farrah, Mislav Balokovic, Daniel Stern +24

We study the geometry of the AGN obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at , using infrared data from Spitzer and Herschel, X-ray data…

astro-ph.GA2016★ 59 cited

Star Formation in Luminous Quasars at 2<z<3

Kathryn Harris, Duncan Farrah, Bernhard Schulz +22

We investigate the relation between star formation rates () and AGN properties in optically selected type 1 quasars at using data from Herschel and the SDSS. W…

astro-ph.CO2013★ 175 cited

Far-infrared Fine-Structure Line Diagnostics of Ultraluminous Infrared Galaxies

Duncan Farrah, Vianney Lebouteiller, Henrik Spoon +16

We present Herschel observations of six fine-structure lines in 25 Ultraluminous Infrared Galaxies at z<0.27. The lines, [O III]52, [N III]57, [O I]63, [N II]122, [O I]145, and [C…

astro-ph.CO2013★ 4 cited

Evidence of Increased UV FeII Emission in Quasars in Candidate Overdense Regions

Kathryn A. Harris, G. M. Williger, L. Haberzettl +6

We present evidence for a skewed distribution of UV FeII emission in quasars within candidate overdense regions spanning spatial scales of ~ 50 Mpc at 1.11 < z < 1.67, compared to…

astro-ph.CO2012★ 149 cited

A structure in the early universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology

Roger G. Clowes, Kathryn A. Harris, Srinivasan Raghunathan +3

A Large Quasar Group (LQG) of particularly large size and high membership has been identified in the DR7QSO catalogue of the Sloan Digital Sky Survey. It has characteristic size (v…

astro-ph.CO2012

The Cluster and Large Scale Environments of Quasars at z<0.9

Kathryn A. Harris

In this thesis, I present an investigation into the environments of quasars with respect to galaxy clusters, and environment evolution with redshift and luminosity. The orientation…