IACTEC líneas: Grandes telescopios

  • Publicación
    Representative galaxy age–metallicity relationships
    The ongoing surveys of galaxies and those for the next generation of telescopes will demand the execution of high-CPU consuming machine codes for recovering...
  • Publicación
    Revised Bolometric Corrections and Interstellar Extinction Coefficients for the ACS and WFPC2 Photometric Systems
    We present extensive tables of bolometric corrections and interstellar extinction coefficients for the WFPC2 and ACS (both WFC and HRC) photometric systems...
  • Publicación
    Rotating stellar populations in the Fornax dSph galaxy
    We present a novel analysis of the internal kinematics of the Fornax dwarf spheroidal galaxy. Our results are based on the largest sample of spectroscopic data...
  • Publicación
    Searching for chemical inhomogeneities in open clusters. Analysis of the CN and CH molecular band strengths in NGC 2158, NGC 2420, NGC 2682, NGC 7789, and Berkeley 29
    Context. The total mass of a cluster, which is the main parameter determining its ability to host more than one stellar generation, may constitute a threshold...
  • Publicación
    SEGUE-2: Old Milky Way Stars Near and Far
    The Sloan Extension for Galactic Understanding and Exploration 2 (SEGUE-2) obtained 128,288 low-resolution spectra (R ~ 1800) of 118,958 unique stars in the...
  • Charla
    Seminario de Instrumentación: Desfile de modelos del Telescopio Solar Europeo (EST)
    La creación y uso de modelos es una parte fundamental de la ingeniería. En esta charla se presentará una visión descriptiva de alto nivel sobre los modelos...
  • Publicación
    Seven young star clusters in the inner region of the Small Magellanic Cloud
    We present CCD photometry in the Washington system C and T1 passbands down to T1 ~ 22 in the fields of L35, L45, L49, L50, L62, L63 and L85, seven poorly...
  • Publicación
    Sodium-Oxygen Anticorrelation and Neutron-capture Elements in Omega Centauri Stellar Populations
    Omega Centauri is no longer the only globular cluster known to contain multiple stellar populations, yet it remains the most puzzling. Due to the extreme way in...