2k citations · 17.8k across the 169 of their papers we have counts for
16 papers · 2 filters
Stellar populations and Lyman-alpha emission from lensed z > 6 galaxies
Daniel Schaerer, Roser Pello
We present results from an SED analysis of two lensed high-z objects, the z=6.56 galaxy HCM6A behind the cluster Abell 370 discovered by Hu et al. (2002) and the triple arc at z~7…
Starbursts at z >~6: from the present to Herschel and ALMA
Daniel Schaerer, Roser Pello
The SED of the lensed z=6.56 galaxy HCM6A behind the cluster Abell 370 has been analysed. We find clear indications for the presence of dust in this galaxy, and we estimate the pro…
The GALEX-VVDS Measurement of the Evolution of the Far-Ultraviolet Luminosity Density and the Cosmic Star Formation Rate
D. Schiminovich, O. Ilbert, S. Arnouts +10
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies…
The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function
S. Arnouts, D. Schiminovich, O. Ilbert +8
We present the first measurement of the galaxy luminosity function at 1500A between 0.2<z<1.2 based on GALEX-VVDS observations (1000 spectroscopic redshifts for galaxies with NUV<2…
Very High-Redshift Lensed Galaxies
R. Pello, D. Schaerer, J. Richard +2
We review in this paper the main results recently obtained on the identification and study of very high-z galaxies usinglensing clusters as natural gravitational telescopes. We pre…
The VVDS data reduction pipeline: introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface
M. Scodeggio, P. Franzetti, B. Garilli +36
The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large a…
Large scale diffuse light in the Coma cluster: a multi-scale approach
C. Adami, E. Slezak, F. Durret +7
We have obtained wide field images of the Coma cluster in the B, V, R and I bands with the CFH12K camera at CFHT. In order to search for large scale diffuse emission, we have appli…
The VIMOS VLT Deep Survey: Computing the two point correlation statistics and associated uncertainties
A. Pollo, B. Meneux, L. Guzzo +43
We are presenting in this paper a detailed account of the methods used to compute the three-dimensional two-point galaxy correlation function in the VIMOS-VLT deep survey (VVDS). W…
The VIMOS-VLT Deep Survey: Evolution of the galaxy luminosity function up to z=2 in first epoch data
O. Ilbert, L. Tresse, E. Zucca +44
We investigate the evolution of the galaxy luminosity function from the VIMOS-VLT Deep Survey (VVDS) from the present to z=2 in five (U, B, V, R and I) rest-frame band-passes. We u…
Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS)
C. Halliday, B. Milvang-Jensen, S. Poirier +12
We present spectroscopic observations of galaxies in 4 clusters at z = 0.7-0.8 and in one cluster at z~0.5 obtained with the FORS2 spectrograph on the VLT as part of the ESO Distan…
Response to "Reanalysis of the spectrum of the z=10 galaxy ISAAC/VLT observations of a lensed galaxy at z=10.0" by Weatherley et al. (astro-ph/0407150)
R. Pello, J. Richard, J. -F. Le Borgne +1
In a recent posting of a submitted paper Weatherley et al. re-analyse the spectroscopic data from our observations of Abell 1835 IR 1916, a galaxy we claimed to be at redshift z=10…
The build-up of the red-sequence in galaxy clusters since z~0.8
G. De Lucia, B. M. Poggianti, A. Aragon-Salamanca +10
We study the rest-frame (U-V) color-magnitude relation in 4 clusters at redshifts 0.7-0.8, drawn from the ESO Distant Cluster Survey. We confirm that red-sequence galaxies in these…
Star-forming galaxies at z ~ 2: a major science case for the EMIR/GOYA survey on GTC
T. Contini, M. Lemoine-Busserolle, R. Pello +2
We present the first results of a project aiming to derive the physical properties of high-redshift lensed galaxies, intrinsically fainter than the Lyman break galaxies currently o…
Observing z>7 sources with the GTC
R. Pello, D. Schaerer, J. Richard +2
We present the first results obtained from our pilot ultra-deep near-IR survey with ISAAC/VLT, aimed at the detection of z>7 sources using lensing clusters as natural Gravitational…
Observing the build-up of the colour-magnitude relation at redshift ~0.8
G. De Lucia, B. M. Poggianti, A. Aragon-Salamanca +11
We analyse the rest-frame (U-V) colour-magnitude relation for 2 clusters at redshift 0.7 and 0.8, drawn from the ESO Distant Cluster Survey. By comparing with the population of red…
VVDS: early results on LSS distribution to z~1.5
O. Le Fèvre, G. Vettolani, D. Maccagni +2
The VIMOS VLT Deep Survey (VVDS) is an on-going program to map the evolution of galaxies, large scale structures and AGNs from the redshift measurement of more than 100000 objects…