activity
19942026
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 32.5k across the 443 of their papers we have counts for

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Showing 2006Show all

15 papers · 1 filter

astro-ph2006

The VIRMOS-VLT Deep Survey: the last 10 billion years of evolution of galaxy clustering

A. Pollo, L. Guzzo, O. Le Fevre +46

We discuss the evolution of clustering of galaxies in the Universe from the present epoch back to z ~ 2, using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS). We presen…

astro-ph2006★ 1k cited

zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

S. J. Lilly, O. Le Fevre, A. Renzini +42

zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to…

astro-ph2006★ 136 cited

531 new spectroscopic redshifts from the CDFS and a test on the cosmological relevance of the GOODS-South field

C. D. Ravikumar, M. Puech, H. Flores +23

(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ <=-20.3) are selected…

astro-ph2006★ 2 cited

Witnessing the build-up of the colour-density relation

O. Cucciati, A. Iovino, C. Marinoni +50

We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS) on scales of R=5 h^(-1)M…

astro-ph2006

The Ages of Early-Type Galaxies at z~1

Sperello di Serego Alighieri, Alessandro Bressan, Lucia Pozzetti

The study of the ages of early-type galaxies and their dependence on galaxy mass and environment is crucial for understanding the formation and early evolution of galaxies. We revi…

astro-ph2006

NIR Follow-Up of the VVDS 02hr Field

S. Temporin, A. Iovino, H. J. McCracken +46

We present a new K-band survey covering 623 arcmin in the VVDS 0226-0430 deep field down to a limiting magnitude K 20.5. We use the spectroscopic sample ex…