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We developed a code for galactic star-counts making use of suitable assumptions on the evolutionary ...
Aims. We present here a new theoretical approach to population synthesis. The aim is to predict colo...
Context. To derive the history of star formation in the Universe a set of calibrated star formation ...
A new method to extract information from color-magnitude diagrams (CMDs) is presented. We employ a R...
The question of how galaxies form and evolve throughout the age of the Universe is at the forefront ...
This paper develops a method for obtaining the star formation histories of a mixed, resolved populat...
To determine the star formation histories of dwarf galaxies we use fossil methods. Compared to the c...
Color-Magnitude Diagrams (CMDs) are plots that compare the magnitudes (luminosities) of stars in dif...
Aims.This paper develops a method for obtaining the star formation histories of a mixed, resolved p...
Context. Most of our knowledge of the stellar component of galaxies is based on the analysis of dist...
We present a new method to determine the star formation and metal enrichment histories of any resolv...
Context. Accurate star formation histories (SFHs) of galaxies are fundamental for understanding the ...
Artículo de publicación ISIContext. Accurate star formation histories (SFHs) of galaxies are fundame...
Objective determination of a star formation history from a colour-magnitude diagram, independently o...
A simple stellar population (SSP) consists of stars with uniform age and metallicity formed by a sin...
We developed a code for galactic star-counts making use of suitable assumptions on the evolutionary ...
Aims. We present here a new theoretical approach to population synthesis. The aim is to predict colo...
Context. To derive the history of star formation in the Universe a set of calibrated star formation ...
A new method to extract information from color-magnitude diagrams (CMDs) is presented. We employ a R...
The question of how galaxies form and evolve throughout the age of the Universe is at the forefront ...
This paper develops a method for obtaining the star formation histories of a mixed, resolved populat...
To determine the star formation histories of dwarf galaxies we use fossil methods. Compared to the c...
Color-Magnitude Diagrams (CMDs) are plots that compare the magnitudes (luminosities) of stars in dif...
Aims.This paper develops a method for obtaining the star formation histories of a mixed, resolved p...
Context. Most of our knowledge of the stellar component of galaxies is based on the analysis of dist...
We present a new method to determine the star formation and metal enrichment histories of any resolv...
Context. Accurate star formation histories (SFHs) of galaxies are fundamental for understanding the ...
Artículo de publicación ISIContext. Accurate star formation histories (SFHs) of galaxies are fundame...
Objective determination of a star formation history from a colour-magnitude diagram, independently o...
A simple stellar population (SSP) consists of stars with uniform age and metallicity formed by a sin...
We developed a code for galactic star-counts making use of suitable assumptions on the evolutionary ...
Aims. We present here a new theoretical approach to population synthesis. The aim is to predict colo...
Context. To derive the history of star formation in the Universe a set of calibrated star formation ...
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