Abstract 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 down to a magnitude IAB=24, in combination with a multi-wavelength dataset from radio to X-rays. We present here the results obtained from the first epoch data, regarding in particular the evolution of the luminosity function.
Zucca E., Ilbert O., Tresse L., Bardelli S., Arnouts S., Zamorani G., et al. (2004). First results from the VIMOS/VLT Deep Survey (VVDS): luminosity functions from z~0 to z~1.5.
First results from the VIMOS/VLT Deep Survey (VVDS): luminosity functions from z~0 to z~1.5
BONGIORNO, ANGELA;GREGORINI, LORETTA;MARANO, BRUNO;
2004
Abstract
Abstract 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 down to a magnitude IAB=24, in combination with a multi-wavelength dataset from radio to X-rays. We present here the results obtained from the first epoch data, regarding in particular the evolution of the luminosity function.File in questo prodotto:
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