Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey
L. Tresse, O. Ilbert, E. Zucca, G. Zamorani, S. Arnouts, S. Bardelli,, and the VVDS team
TL;DR
This paper analyzes the evolution of galaxy populations across a broad redshift range using the VIMOS VLT Deep Survey, focusing on properties like type, morphology, environment, and luminosity.
Contribution
It provides new insights into galaxy evolution by utilizing a comprehensive spectroscopic sample spanning from redshift 5 to 0.
Findings
Evolution of galaxy types and morphologies over cosmic time
Correlation between environment and galaxy properties
Luminosity-dependent galaxy evolution patterns
Abstract
The VIMOS VLT Deep Survey is a unique I-selected spectroscopic sample to study galaxies all the way from z=5 to z=0. We recapitulate the first results about the evolution of the galaxy populations as a function of type, morphology, environment and luminosity.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Adaptive optics and wavefront sensing