Tipo de publicación: Sin árbitro

  • Publicación
    Stellar astrophysics for the local group : VIII Canary Islands Winter School of Astrophysics
    With the recent advent of large, ground-based telescopes and space telescopes, it is now possible to study in detail stars outside our galaxy--in neighboring...
  • Publicación
    Stellar atmospheres. Beyond classical models
    Not Available
  • Publicación
    Stellar atmospheric parameters in MILES library (Cenarro+, 2007)
    We present a homogeneous set of stellar atmospheric parameters (Teff, logg, [Fe/H]) for MILES, a new spectral stellar library covering the range {lambda}{lambda...
  • Publicación
    Stellar atmospheric parameters of CARMENES GTO M dwarfs with spectral synthesis and SteParSyn
    We aim to review the spectral synthesis technique to derive the stellar atmospheric parameters (T eff, log g, and [Fe/H]) of 348 M dwarfs in light of the...
  • Publicación
    Stellar atmospheric parameters of CARMENES GTO M-dwarfs with spectral synthesis and SteParSyn
    We aim to review the spectral synthesis technique to derive the stellar atmospheric parameters (T eff, log g, and [Fe/H]) of 348 M dwarfs in light of the...
  • Publicación
    Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra
    With the aim of using classic spectroscopic methods with high resolution and high signal-to-noise ratio in the NIR spectral window, we made a selection of 66...
  • Publicación
    Stellar Atmospheric Parameters: The Four-Step Program and Gaia's Radial Velocity Spectrometer
    The determination of atmospheric parameters is the first and most fundamental step in the analysis of a stellar spectrum. Current and forthcoming surveys...
  • Publicación
    Stellar black holes at the dawn of the Universe: cosmological implications
    Not Available
  • Publicación
    Stellar Cluster Abundances from APOGEE Commissioning Spectra
    The Apache Point Observatory Galactic Evolution Experiment (APOGEE) will undertake an H-band (1.52-1.68 micron) spectroscopic survey of 1E5 red giant stars...