A theoretical approach relying on evolutionary population synthesis models could help refining the search criteria in deep galaxy surveys on the basis of a better knowledge of the expected apparent photometric properties of high-redshift objects. The following is a brief discussion reviewing some relevant aspects of the question in order to allow a more critical appraisal to primeval galaxy recognition
We analyze the photometric information contained in individual pixels of galaxies in the Hubble Deep...
Photometric redshifts are estimated on the basis of template scenarios with the help of the code ZPE...
International audience Aims: We compare six popularly used evolutionary population synthesis (EPS) m...
The basic assumptions behind Population Synthesis and Spectral Evolution models are reviewed. The nu...
We present our chemically consistent GALEV Evolutionary Synthesis models for galaxies and point out ...
We present a Bayesian hierarchical framework to analyze photometric galaxy survey data with stellar ...
Aims. We compare six popularly used evolutionary population synthesis (EPS) models by fitting the f...
We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in e...
This thesis focuses on the selection and study of galaxies based on their star formation activity at...
The original publication is available at www.springerlink.com . Copyright Springer DOI : 10.1023/A:1...
This thesis explores the evolution of galaxies from the onset of star formation shortly after the Bi...
In this paper, we explore the plausible luminosity evolution of early-type galaxies in different cos...
The ultraviolet luminosity evolution of star-forming galaxies is explored from the theoretical point...
Increasingly good statistical data on the galaxy population at high and low redshift enable the deve...
Photometric redshifts are estimated on the basis of template scenarios with the help of the code Z-...
We analyze the photometric information contained in individual pixels of galaxies in the Hubble Deep...
Photometric redshifts are estimated on the basis of template scenarios with the help of the code ZPE...
International audience Aims: We compare six popularly used evolutionary population synthesis (EPS) m...
The basic assumptions behind Population Synthesis and Spectral Evolution models are reviewed. The nu...
We present our chemically consistent GALEV Evolutionary Synthesis models for galaxies and point out ...
We present a Bayesian hierarchical framework to analyze photometric galaxy survey data with stellar ...
Aims. We compare six popularly used evolutionary population synthesis (EPS) models by fitting the f...
We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in e...
This thesis focuses on the selection and study of galaxies based on their star formation activity at...
The original publication is available at www.springerlink.com . Copyright Springer DOI : 10.1023/A:1...
This thesis explores the evolution of galaxies from the onset of star formation shortly after the Bi...
In this paper, we explore the plausible luminosity evolution of early-type galaxies in different cos...
The ultraviolet luminosity evolution of star-forming galaxies is explored from the theoretical point...
Increasingly good statistical data on the galaxy population at high and low redshift enable the deve...
Photometric redshifts are estimated on the basis of template scenarios with the help of the code Z-...
We analyze the photometric information contained in individual pixels of galaxies in the Hubble Deep...
Photometric redshifts are estimated on the basis of template scenarios with the help of the code ZPE...
International audience Aims: We compare six popularly used evolutionary population synthesis (EPS) m...