activity
19952009
most citedThe spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe

488 citations · 1.5k across the 21 of their papers we have counts for

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Showing 2004 · astro-phShow all

6 papers · 2 filters

astro-ph2004

XMM-Newton EPIC observations of the ultraluminous X-ray source NGC 5204 X-1

T. P. Roberts, R. S. Warwick, M. J. Ward +2

We present the results of two XMM-Newton observations of the ultraluminous X-ray source (ULX) NGC 5204 X-1. The EPIC spectra are well-fit by the standard spectral model of a black-…

astro-ph2004

The Phoenix Deep Survey: spectroscopic catalog

J. Afonso, A. Georgakakis, C. Almeida +4

The Phoenix Deep Survey is a multi-wavelength survey based on deep 1.4 GHz radio imaging, reaching well into the sub-100 microJy level. One of the aims of this survey is to charact…

astro-ph2004

A Panoramic Halpha Imaging Survey of the z=0.4 cluster Cl0024.0+1652 with Subaru

Tadayuki Kodama, Michael Balogh, Ian Smail +2

We employ panoramic, multicolour (BRz') and narrow-band Halpha imaging of the cluster Cl0024.0+1652 (z=0.39) from Subaru covering a ~30 arcmin field, to determine cluster membershi…

astro-ph20047 cited

Disk Galaxy Rotation Curves in Triaxial CDM Halos

E. Hayashi, J. F. Navarro, A. Jenkins +7

We use N-body hydrodynamical simulations to study the structure of disks in triaxial potentials resembling CDM halos. Our analysis focuses on the accuracy of the dark mass distribu…

astro-ph2004

The Observed and Predicted Spatial Distribution of Milky Way Satellite Galaxies

B. Willman, F. Governato, J. J. Dalcanton +2

We review evidence that the census of Milky Way satellites similar to those known may be incomplete at low latitude due to obscuration and in the outer halo due to a decreasing sen…

astro-ph2004

Quenching Cluster Cooling Flows with Recurrent Hot Plasma Bubbles

Claudio Dalla Vecchia, Richard Bower, Tom Theuns +3

The observed cooling rate of hot gas in clusters is much lower than that inferred from the gas density profiles. This suggests that the gas is being heated by some source. We use a…