activity
19972004
most citedStellar masses, star formation rates, metallicities and AGN properties for 200,000 galaxies in the SDSS Data Release Two (DR2)

15 citations · 15 across the 2 of their papers we have counts for

collaborators

7 papers

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

The Star Formation Histories of Local Galaxies: Continuous or Intermittent?

Guinevere Kauffmann, Stephane Charlot, Michael L. Balogh

We explore a model in which efficient star formation in galaxies is triggered by merging satellites. We show that the merger/interaction rates predicted by hierarchical galaxy form…

astro-ph1999

The formation and evolution of supermassive black holes and their host galaxies

Martin G. Haehnelt, Guinevere Kauffmann

We discuss constraints on the assembly history of supermassive black holes from the observed remnant black holes in nearby galaxies and from the emission caused by accretion onto t…

astro-ph1999

Probing Star Formation Timescales in Elliptical Galaxies

Daniel Thomas, Guinevere Kauffmann

In models of galaxy formation in a hierarchical Universe, elliptical galaxies form through the merging of smaller disk systems. These models yield a number of testable predictions…

astro-ph1998

Evolution of Elliptical Galaxies in a Hierarchical Universe

Guinevere Kauffmann, Stephane Charlot

In hierarchical models of galaxy formation, ellipticals form from the merging of disk galaxies drawn together by gravity as their surrounding dark halos coalesce. Using semi-analyt…