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 2003 · astro-phShow all

9 papers · 2 filters

astro-ph2003

Galaxy Evolution in Three dimensions : Time, Space and Mass

Tadayuki Kodama, Richard Bower, Philip Best +3

There are three major axes to describe the evolution of galaxies, namely, time (redshift), space (environment) and mass (stellar mass). In this article, one topic each will be pres…

astro-ph20031 cited

The very high state accretion disk structure from the galactic black hole transient XTE J1550-564

Aya Kubota, Chris Done

The 1998 outburst of the bright Galactic black hole binary system XTE J1550-564 was used to constrain the accretion disc structure in the strongly Comptonised very high state spect…

astro-ph2003

Simulating Chandra observations of galaxy clusters

A. Gardini, E. Rasia, P. Mazzotta +3

Numerical hydro-N-body simulations are very important tools for making theoretical predictions for the formation of galaxy clusters. They show that the atmospheres of clusters of g…

astro-ph2003

Near-Infrared Colors of Submillimeter-Selected Galaxies

D. T. Frayer, N. A. Reddy, L. Armus +3

We report on deep near-infrared (NIR) observations of submillimeter-selected galaxies (SMGs) with the Near Infrared Camera (NIRC) on the Keck I telescope. We have identified K-band…

astro-ph2003

The Inner Structure of LCDM Halos II: Halo Mass Profiles and LSB Rotation Curves

E. Hayashi, J. F. Navarro, C. Power +6

We use a set of high-resolution cosmological N-body simulations to investigate the inner mass profile of galaxy-sized cold dark matter (CDM) halos. These simulations extend the tho…

astro-ph2003

Extremely red galaxies in the Phoenix Deep Survey

A. M. Hopkins, J. Afonso, A. Georgakakis +3

The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Here we present…