We present a homogeneous set of stellar atmospheric parameters Teff, log g, [Fe/H] for MILES, a new spectral stellar library covering the range 3525 - 7500 angstrom at 2.3 angstrom (FWHM) spectral resolution. The library consists of 985 stars spanning a large range in atmospheric parameters, from super metal-rich, cool stars to hot, metal-poor stars. The spectral resolution, spectral type coverage and number of stars represent a substantial improvement over previous libraries used in population synthesis models. The atmospheric parameters that we present here are the result of a previous, extensive compilation from the literature. In order to construct a homogeneous dataset of atmospheric parameters we have taken the sample of stars of Soub...
Context. The detection and subsequent characterisation of exoplanets are intimately linked to the ch...
We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at the Obse...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
Theoretical stellar libraries have been increasingly used to overcome limitations of empirical libra...
Studies of Galactic chemical, and dynamical evolution in the solar neighborhood depend on the availa...
Context. The X-shooter Spectral Library (XSL) is an empirical stellar library at medium spectral res...
We present the single stellar population (SSP) synthesis results of our new synthetic stellar atmosp...
A new stellar library developed for stellar population synthesis modeling is presented. The library ...
Context. The detection and subsequent characterisation of exoplanets are intimately linked to the ch...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
Context. The detection and subsequent characterisation of exoplanets are intimately linked to the ch...
We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at the Obse...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
Theoretical stellar libraries have been increasingly used to overcome limitations of empirical libra...
Studies of Galactic chemical, and dynamical evolution in the solar neighborhood depend on the availa...
Context. The X-shooter Spectral Library (XSL) is an empirical stellar library at medium spectral res...
We present the single stellar population (SSP) synthesis results of our new synthetic stellar atmosp...
A new stellar library developed for stellar population synthesis modeling is presented. The library ...
Context. The detection and subsequent characterisation of exoplanets are intimately linked to the ch...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
Context. The detection and subsequent characterisation of exoplanets are intimately linked to the ch...
We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at the Obse...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...