activity
19942009
most citedThe redshift dependence of the structure of massive LCDM halos

510 citations · 5.9k across the 44 of their papers we have counts for

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Showing 2004 · astro-phShow all

11 papers · 2 filters

astro-ph2004

The Third Data Release of the Sloan Digital Sky Survey

K. Abazajian et al.

This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through June 2003, includes imaging data in five bands ov…

astro-ph2004

Pure Luminosity Evolution Models: Too Few Massive Galaxies at Intermediate and High Redshift

M. G. Kitzbichler, S. D. M. White

We compare pure luminosity evolution (PLE) models with recent data at low and high redshift. These models assume that massive galaxies were assembled and formed most of their stars…

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-ph200415 cited

Stellar masses, star formation rates, metallicities and AGN properties for 200,000 galaxies in the SDSS Data Release Two (DR2)

Jarle Brinchmann, Stephane Charlot, Timothy M. Heckman +3

By providing homogeneous photometric and spectroscopic data of high quality for very large and objectively selected samples of galaxies, the Sloan Digital Sky Survey allows statist…

astro-ph2004

Present-Day Growth of Black Holes and Bulges: the SDSS Perspective

Timothy M. Heckman, Guinevere Kauffmann, Jarle Brinchmann +3

We investigate the accretion-driven growth of supermassive black holes in the low-redshift Universe using 23,000 ``Type 2'' AGN and the complete sample of 123,000 galaxies in the S…

astro-ph2004

Galaxies and subhaloes in LCDM galaxy clusters

Liang Gao, Gabriella De Lucia, Simon D. M. White +1

We combine 10 high resolution resimulations of cluster--sized dark haloes with semi--analytic galaxy formation modelling in order to compare the number density and velocity dispers…