activity
19952025
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 23.4k across the 217 of their papers we have counts for

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Showing 2006Show all

13 papers · 1 filter

astro-ph2006★ 151 cited

Photometric Redshifts of Galaxies in COSMOS

B. Mobasher, P. Capak, N. Z. Scoville +26

We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the optio…

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★ 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 VVDS-VLA Deep Field: III. GMRT observations at 610 MHz and the radio spectral index properties of the sub-mJy population

M. Bondi, P. Ciliegi, T. Venturi +12

We present the low frequency (610 MHz) radio source counts of the VVDS-VLA field and investigate the radio spectral index properties of the sub-mJy population. We use new deep (r.m…

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…