We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at the Observatoire de Haute-Provence. 52 orders of the echelle spectra have been carefully fitted together to provide continuous, high-resolution spectra in the wavelength range $\lambda\lambda = 410{-}680$ nm. The archive provides a large coverage of the space of atmospheric parameters: Teff from 3700 K to 13 600 K, $\log g$ from 0.03 to 5.86 and [Fe/H] from -2.8 to +0.7. At the nominal resolution, $R=42 000$, the mean signal-to-noise ratio is 150 per pixel. The spectra given at this resolution are normalized to their pseudo-continuum and are intended to serve for abundance studies, spectral classification and tests of stellar atmosphere mode...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
Aims. Synthetic spectra are needed to determine fundamental stellar and wind parameters of all types...
Context. Empirical stellar spectral libraries have applications in both extragalactic and stellar st...
We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at Observato...
We present a homogeneous set of stellar atmospheric parameters Teff, log g, [Fe/H] for MILES, a new ...
Libraries of stellar spectra have been used for a large variety of science cases, including populati...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
We present a review of open-source data for stellar spectroscopy investigations. It includes lists o...
We present a library of Utrecht echelle spectrograph (UES) observations of a sample of F, G, K and M...
We present an Atlas of high resolution (resolving power $\lambda/\Delta\lambda = 250~000$) syntheti...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
A sample of 37 stars of luminosity classes I, III, V, including few SMR stars observed in the H band...
Abstract. We present an Atlas of high resolution (re-solving power = = 250 000) synthetic spectra ...
We present a library of Penn State Fiber Optic Echelle (FOE) observations of a sample of field stars...
We present an Echelle+CCD high resolution spectroscopic atlas (0.25 Å/pix dispersion, 0.43 Å FWHM re...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
Aims. Synthetic spectra are needed to determine fundamental stellar and wind parameters of all types...
Context. Empirical stellar spectral libraries have applications in both extragalactic and stellar st...
We present a database of 908 spectra of 709 stars obtained with the ELODIE spectrograph at Observato...
We present a homogeneous set of stellar atmospheric parameters Teff, log g, [Fe/H] for MILES, a new ...
Libraries of stellar spectra have been used for a large variety of science cases, including populati...
We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for MILES, a n...
We present a review of open-source data for stellar spectroscopy investigations. It includes lists o...
We present a library of Utrecht echelle spectrograph (UES) observations of a sample of F, G, K and M...
We present an Atlas of high resolution (resolving power $\lambda/\Delta\lambda = 250~000$) syntheti...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
A sample of 37 stars of luminosity classes I, III, V, including few SMR stars observed in the H band...
Abstract. We present an Atlas of high resolution (re-solving power = = 250 000) synthetic spectra ...
We present a library of Penn State Fiber Optic Echelle (FOE) observations of a sample of field stars...
We present an Echelle+CCD high resolution spectroscopic atlas (0.25 Å/pix dispersion, 0.43 Å FWHM re...
A new stellar library developed for stellar population synthesis modelling is presented. The library...
Aims. Synthetic spectra are needed to determine fundamental stellar and wind parameters of all types...
Context. Empirical stellar spectral libraries have applications in both extragalactic and stellar st...