activity
19942026
most citedA Universal Density Profile from Hierarchical Clustering

9.9k citations · 112.1k across the 575 of their papers we have counts for

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Showing 2010Show all

21 papers · 1 filter

astro-ph.CO2010★ 32 cited

Galaxy And Mass Assembly (GAMA): Galaxies at the faint end of the Halpha luminosity function

S. Brough, A. M. Hopkins, R. G. Sharp +30

We present an analysis of the properties of the lowest Halpha-luminosity galaxies (L_Halpha<4x10^32 W; SFR<0.02 Msun/yr) in the Galaxy And Mass Assembly (GAMA) survey. These galaxi…

astro-ph.CO2010★ 19 cited

Star formation trends in high-redshift galaxy surveys: the elephant or the tail?

Martin Stringer, Shaun Cole, Carlos S. Frenk +1

Star formation rate and accummulated stellar mass are two fundamental physical quantities that describe the evolutionary state of a forming galaxy. Two recent attempts to determine…

astro-ph.CO2010★ 191 cited

The evolution of AGN across cosmic time: what is downsizing?

N. Fanidakis, C. M. Baugh, A. J. Benson +7

We use a coupled model of the formation and evolution of galaxies and black holes (BH) to study the evolution of active galactic nuclei (AGN) in a cold dark matter universe. The mo…

astro-ph.CO2010★ 13 cited

Which halos host Herschel-ATLAS galaxies in the local Universe?

Qi Guo, Shaun Cole, Cedric G. Lacey +40

We measure the projected cross-correlation between low redshift (z < 0.5) far-IR selected galaxies in the SDP field of the Herschel-ATLAS (H-ATLAS) survey and optically selected ga…

astro-ph.CO2010★ 5 cited

The similarity of observed X-ray coronae associated with L* disc and elliptical galaxies

Robert A. Crain, Ian G. McCarthy, Joop Schaye +2

The existence of hot, X-ray luminous gaseous coronae surrounding present day L* galaxies is a generic prediction of galaxy formation theory in the cold dark matter cosmogony. While…

astro-ph.GA2010★ 27 cited

A Two-Point Correlation Function For Galactic Halo Stars

A. P. Cooper, S. Cole, C. S. Frenk +1

We describe a correlation function statistic that quantifies the amount of spatial and kinematic substructure in the stellar halo. We test this statistic using model stellar halo r…