2 citations · 2 across the 5 of their papers we have counts for
9 papers · 1 filter
Studying the evolution of large-scale structure with the VIMOS-VLT Deep Survey
L. Guzzo, O. Le Fevre, B. Meneux +16
The VIMOS-VLT Deep Survey (VVDS) currently offers a unique combination of depth, angular size and number of measured galaxies among surveys of the distant Universe: ~ 11,000 spectr…
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…
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…
The VLT-VIMOS Mask Preparation Software
D. Bottini, B. Garilli, D. Maccagni +34
VIMOS (VIsible Multi-Object Spectrograph) is a multi-object imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Obse…
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…
AgapeZ1: a Large Amplification Microlensing Event or an Odd Variable Star Towards the Inner Bulge of M31
R. Ansari, M. Auriere, P. Baillon +14
AgapeZ1 is the brightest and the shortest duration microlensing candidate event found in the Agape data. It occured only 42" from the center of M31. Our photometry shows that the h…