I present an overview of empirical stellar spectral libraries, their uses, and (briefly) their history. I focus primarily on their utility for understanding the stellar populations of composite stellar systems, but I show examples of their use for topics ranging from the determination of atmospheric parameters of stars outside the libraries to calibration of stellar atmosphere models to stellar radial velocities. I end by presenting the ``state of the art'' of available stellar spectral libraries focused on stellar population synthesis and what still needs to be done in the near future
I present the results of an investigation into the spectral properties of stars and galaxies. Firstl...
Astronomical objects are generally studied through observation-to-model comparisons. Galaxies are co...
Libraries of stellar spectra are fundamental tools for the study of stellar populations, and both em...
I present an overview of empirical stellar spectral libraries, their uses, and (briefly) their histo...
Grids of stellar spectra are extensively used in astrophysics in a range of applications, from deriv...
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...
I describe very briefly the new libraries of empirical spectra of stars covering wide ranges of valu...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
International audienceStellar population synthesis (SPS) models are invaluable to study star cluster...
We have computed a theoretical library of stellar spectra, from Near-UV to Near-IR, with varying abu...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
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 ...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
I present the results of an investigation into the spectral properties of stars and galaxies. Firstl...
Astronomical objects are generally studied through observation-to-model comparisons. Galaxies are co...
Libraries of stellar spectra are fundamental tools for the study of stellar populations, and both em...
I present an overview of empirical stellar spectral libraries, their uses, and (briefly) their histo...
Grids of stellar spectra are extensively used in astrophysics in a range of applications, from deriv...
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...
I describe very briefly the new libraries of empirical spectra of stars covering wide ranges of valu...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
International audienceStellar population synthesis (SPS) models are invaluable to study star cluster...
We have computed a theoretical library of stellar spectra, from Near-UV to Near-IR, with varying abu...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
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 ...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
I present the results of an investigation into the spectral properties of stars and galaxies. Firstl...
Astronomical objects are generally studied through observation-to-model comparisons. Galaxies are co...
Libraries of stellar spectra are fundamental tools for the study of stellar populations, and both em...