In this paper we show how evolution strategies (ES) are successfully applied to the problem of fitting line profiles of stellar spectra, which provides a reliable decomposition. Using a stellar spectrum as input, we implemented an evolution strategy to find its components: continuos spectrum and spectral lines. In our experiments we used Gaussian functions to match spectral lines and three different equations to represent the continuos spectrum. We applied this method to simulated and real spectra
A new method of analysing spectra, based on a genetic algorithm, is presented. The algorithm reconst...
International audienceThe study of stellar populations in galaxies is entering a new era with the av...
International audienceContext. The homogenization of the stellar parameters is an important goal for...
Current surveys from modern astronomical observatories contain a huge amount of data; in particular,...
This animation illustrates the decomposition of an ensemble of absorption lines into individual mode...
In this work we employ Evolution Strategies (ES) to automatically extract a set of physical paramete...
Abstract. The observation of evolved stars in selected evolutionary stages allow us to track the evo...
We present the single stellar population (SSP) synthesis results of our new synthetic stellar atmosp...
The Evolutionary spectrum inversion and analysis (Especia) file set provides ISO C++ code for the in...
The goal of population spectral synthesis (pss; also referred to as inverse, semi-empirical evolutio...
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar...
Context. The homogenization of the stellar parameters is an important goal for large observational s...
Abstract. | When analyzing any wavelength region, stellar spectroscopists must deal with the multitu...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
Aims. We provide an easy-to-use full-spectrum fitting package and explore its applications to (i)...
A new method of analysing spectra, based on a genetic algorithm, is presented. The algorithm reconst...
International audienceThe study of stellar populations in galaxies is entering a new era with the av...
International audienceContext. The homogenization of the stellar parameters is an important goal for...
Current surveys from modern astronomical observatories contain a huge amount of data; in particular,...
This animation illustrates the decomposition of an ensemble of absorption lines into individual mode...
In this work we employ Evolution Strategies (ES) to automatically extract a set of physical paramete...
Abstract. The observation of evolved stars in selected evolutionary stages allow us to track the evo...
We present the single stellar population (SSP) synthesis results of our new synthetic stellar atmosp...
The Evolutionary spectrum inversion and analysis (Especia) file set provides ISO C++ code for the in...
The goal of population spectral synthesis (pss; also referred to as inverse, semi-empirical evolutio...
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar...
Context. The homogenization of the stellar parameters is an important goal for large observational s...
Abstract. | When analyzing any wavelength region, stellar spectroscopists must deal with the multitu...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
Aims. We provide an easy-to-use full-spectrum fitting package and explore its applications to (i)...
A new method of analysing spectra, based on a genetic algorithm, is presented. The algorithm reconst...
International audienceThe study of stellar populations in galaxies is entering a new era with the av...
International audienceContext. The homogenization of the stellar parameters is an important goal for...