2k citations · 20.1k across the 181 of their papers we have counts for
9 papers · 1 filter
The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- VI. 350 micron mapping of submillimetre galaxies
Kristen Coppin, Mark Halpern, Douglas Scott +24
A follow-up survey using the Submillimetre High-Angular Resolution Camera (SHARC-II) at 350 microns has been carried out to map the regions around several 850 micron-selected sourc…
The assembly bias of dark matter haloes to higher orders
R. E. Angulo, C. M. Baugh, C. G. Lacey
We use an extremely large volume (), high resolution N-body simulation to measure the higher order clustering of dark matter haloes as a function of mass an…
A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
Michael Rauch, Martin Haehnelt, Andrew Bunker +10
We have conducted a long slit search for low surface brightness Lyman-alpha emitters at redshift 2.67 < z < 3.75. A 92 hour long exposure with VLT/FORS2 down to a 1-sigma surface b…
Ram pressure stripping the hot gaseous halos of galaxies in groups and clusters
Ian G. McCarthy, Carlos S. Frenk, Andreea S. Font +5
We use a large suite of carefully controlled full hydrodynamic simulations to study the ram pressure stripping of the hot gaseous halos of galaxies as they fall into massive groups…
Luminous Red Galaxies in hierarchical cosmologies
C. Almeida, C. M. Baugh, D. A. Wake +4
Luminous red galaxies (LRGs) are much rarer and more massive than L* galaxies. Coupled with their extreme colours, LRGs therefore provide a demanding testing ground for the physics…
Narrow-band surveys for very high redshift Lyman-alpha emitters
Kim K. Nilsson, Alvaro Orsi, Cedric G. Lacey +2
Context: Many current and future surveys aim to detect the highest redshift (z >~ 7) sources through their Lyman-alpha (Ly-alpha) emission, using the narrow-band imaging method. Ho…
The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5
P. A. Oesch, M. Stiavelli, C. M. Carollo +14
We present the UDF05 project, a HST Large Program of deep ACS (F606W, F775W, F850LP) and NICMOS (F110W, F160W) imaging of three fields, two of which coincide with the NICP1-4 NICMO…
Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
C. G. Lacey, C. M. Baugh, C. S. Frenk +3
We present predictions for the evolution of the galaxy luminosity function, number counts and redshift distributions in the IR based on the Lambda-CDM cosmological model. We use th…
Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
Ian G. McCarthy, Richard G. Bower, Michael L. Balogh +6
(Abridged) The thermal history of the intracluster medium (ICM) is complex. Heat input from cluster mergers, AGN, and galaxy winds offsets and may even halt the cooling of the ICM.…