Add to ORKGIn the last decade, optical and near-infrared surveys played a crucial role to unveil and decipher the main evolutionary trends which characterize galaxy evolution over a wide interval of cosmic time. The purpose of this paper is to review some of the major results on the nature and properties of the galaxy populations identified at cosmological distances in the optical/near--IR, and on their star formation, mass assembly and metallicity cosmic histories
International audienceDetermination of the star formation rate can be done using mid-IR photometry o...
The new generation of 8 to 10-meter class telescopes opens exciting new possibilities for observatio...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...
In the last decade, optical and near-infrared surveys played a crucial role to unveil and decipher t...
none1noNear-infrared surveys provide one of the best opportunities to investigate the cosmic evoluti...
Over the last decade optical spectroscopic surveys have characterized the low redshift galaxy popula...
The star formation history of galaxies is the primary influence on galaxy evolution, and hence the e...
Evolution of the content and light of galaxies are studied to determine their significance for cosmo...
We discuss the constraints set on galaxy evolution by a variety of data from deep extragalactic surv...
It has been a big challenge to study galaxy formation and evolution in an observational manner at th...
This thesis explores the properties of distant galaxies in the Universe, in particular their redshif...
One of the major questions in observational cosmology is how galaxies formed and how they evolved. I...
Infrared surveys provide essential insights on galaxy evolution. If near-IR studies suggest a mild e...
The analysis of stellar populations provides key insight into the formation and evolution of galaxie...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
International audienceDetermination of the star formation rate can be done using mid-IR photometry o...
The new generation of 8 to 10-meter class telescopes opens exciting new possibilities for observatio...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...
In the last decade, optical and near-infrared surveys played a crucial role to unveil and decipher t...
none1noNear-infrared surveys provide one of the best opportunities to investigate the cosmic evoluti...
Over the last decade optical spectroscopic surveys have characterized the low redshift galaxy popula...
The star formation history of galaxies is the primary influence on galaxy evolution, and hence the e...
Evolution of the content and light of galaxies are studied to determine their significance for cosmo...
We discuss the constraints set on galaxy evolution by a variety of data from deep extragalactic surv...
It has been a big challenge to study galaxy formation and evolution in an observational manner at th...
This thesis explores the properties of distant galaxies in the Universe, in particular their redshif...
One of the major questions in observational cosmology is how galaxies formed and how they evolved. I...
Infrared surveys provide essential insights on galaxy evolution. If near-IR studies suggest a mild e...
The analysis of stellar populations provides key insight into the formation and evolution of galaxie...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
International audienceDetermination of the star formation rate can be done using mid-IR photometry o...
The new generation of 8 to 10-meter class telescopes opens exciting new possibilities for observatio...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...