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20012026
most citedFrom dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology

1.2k citations · 10.6k across the 180 of their papers we have counts for

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Showing 2009Show all

15 papers · 1 filter

astro-ph.CO2009★ 3 cited

Metallicity distributions in and around galaxies

Gabriella De Lucia

Metals are found in all baryonic phases and environments, and our knowledge of their distribution `in and around galaxies' has significantly improved over the past few years. Theor…

astro-ph.CO2009★ 129 cited

Stellar Ages and Metallicities of Central and Satellite Galaxies: Implications for Galaxy Formation and Evolution

Anna Pasquali, Anna Gallazzi, Fabio Fontanot +4

Using a large SDSS galaxy group catalogue, we study how the stellar ages and metallicities of central and satellite galaxies depend on stellar mass and halo mass. We find that sate…

astro-ph.GA2009★ 129 cited

Cluster Galaxies Die Hard

Simone M. Weinmann, Guinevere Kauffmann, Anja von der Linden +1

We investigate how the specific star formation rates of galaxies of different masses depend on cluster-centric radius and on the central/satellite dichotomy in both field and clust…

astro-ph.CO2009★ 40 cited

The VIMOS VLT Deep Survey: the group catalogue

O. Cucciati, C. Marinoni, A. Iovino +39

[Abridged] We present a homogeneous and complete catalogue of optical groups identified in the purely flux limited (17.5<=I<=24.0) VIMOS-VLT Deep Survey (VVDS). We use mock catalog…

astro-ph.CO2009★ 46 cited

Photometric redshifts and cluster tomography in the ESO Distant Cluster Survey

R. Pello, G. Rudnick, G. De Lucia +17

This paper reports the results obtained on the photometric redshifts measurement and accuracy, and cluster tomography in the ESO Distant Cluster Survey (EDisCS) fields. Photometric…

astro-ph.CO2009★ 53 cited

Evolution of the Early-Type Galaxy Fraction in Clusters since z = 0.8

Luc Simard, Douglas Clowe, Vandana Desai +13

We study the morphological content of a large sample of high-redshift clusters to determine its dependence on cluster mass and redshift. Quantitative morphologies are based on bulg…