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19942005
most citedStellar masses, star formation rates, metallicities and AGN properties for 200,000 galaxies in the SDSS Data Release Two (DR2)

15 citations · 22 across the 4 of their papers we have counts for

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27 papers · 1 filter

astro-ph2005

Supernova outflows in galaxy formation

Cecilia Scannapieco, Patricia B. Tissera, Simon D. M. White +1

We investigate the generation of galactic outflows by supernova feedback in the context of SPH cosmological simulations. We use a modified version of the code GADGET-2 which includ…

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-ph2003

Evolution of galaxies in clusters: semi-analytic models and observations

Gabriella De Lucia, Guinevere Kauffmann, Simon D. M. White

We present two different projects. The first one is related to the development of a semi-analytic model to follow the formation, the evolution and chemical enrichment of cluster ga…

astro-ph2001

On the phase-space structure of the Milky Way dark-matter halo

Amina Helmi, Volker Springel, Simon D. M. White

We analyse a high resolution simulation of the formation of a cluster's dark-matter halo in a CDM cosmology (Springel et al. 2001). The resolution achieved allows us to map the…

astro-ph2001

Cosmic Shear from STIS Pure Parallels: Analysis

H. Haemmerle, J. -M. Miralles, P. Schneider +5

The measurement of cosmic shear requires deep imaging with high image quality on many lines of sight to sample the statistics of large-scale structure. The expected distortion of g…