1.2k citations · 26.8k across the 398 of their papers we have counts for
6 papers · 1 filter
Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
S. de la Torre, B. Meneux, G. De Lucia +37
This paper presents a detailed comparison between high-redshift observations from the VIMOS-VLT Deep Survey (VVDS) and predictions from the Munich semi-analytical model of galaxy f…
The VIMOS VLT Deep Survey: the contribution of minor mergers to the growth of L_B >= L*_B galaxies since z ~ 1 from spectroscopically identified pairs
C. López-Sanjuan, O. Le Fèvre, L. de Ravel +14
In this work we measure the merger fraction, f_m, of L_B >= L*_B galaxies in the VVDS-Deep spectroscopic Survey. We define kinematical close pairs as those galaxies with a separati…
The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
Asantha Cooray, Steve Eales, Scott Chapman +247
A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwa…
The WIRCAM Deep Infrared Cluster Survey I: Groups and Clusters at z > 1.1
R. M. Bielby, A. Finoguenov, M. Tanaka +12
We use CFHTLS deep optical data, WIRCam Deep Survey (WIRDS) NIR data and XMM data to identify z>1.1 clusters in the CFHTLS D1 and D4 fields. Counterparts to such clusters can not b…
The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z 1
U. Abbas, S. de la Torre, O. Le Fèvre +47
We model the evolution of the mean galaxy occupation of dark-matter halos over the range , using the data from the VIMOS-VLT Deep Survey (VVDS). The galaxy projected cor…
The VIMOS VLT Deep Survey: Star Formation Rate Density of Lya emitters from a sample of 217 galaxies with spectroscopic redshifts 2<z<6.6
P. Cassata, O. Le Fevre, B. Garilli +18
Aims. The aim of this work is to study the contribution of the Ly-a emitters (LAE) to the star formation rate density (SFRD) of the Universe in the interval 2<z<6.6. Methods. We as…