Publication type: Non-refereed

  • Publication
    CT1 photometry of 5 SMC star clusters (Piatti+, 2007)
    The CCD images were obtained using the 1.54-m Danish telescope at the European Southern Observatory (ESO) on La Silla, equipped with the Danish Faint Object...
  • Publication
    CT1 photometry of 7 young SMC star clusters (Piatti+, 2008)
    The observations of the cluster sample were obtained with the Danish Faint Object Spectrograph and Camera (DFOSC) on the 1.54-m Danish Telescope at the European...
  • Publication
    Cu and Zn Abundances in Metal Poor Stars
    We present Cu and Zn abundances for a sample of 30 stars spanning a metallicity range between solar and [Fe/H]=-3. LTE abundances were obtained using Kurucz...
  • Publication
    Cu and Zn Abundances in Metal Poor Stars
    We present Cu and Zn abundances for a sample of 30 stars spanning a metallicity range between solar and [Fe/H]=-3. LTE abundances were obtained using Kurucz...
  • Publication
    Cu and Zn abundances in metal-poor stars
    We present Cu and Zn abundances for a sample of 30 stars spanning a metallicity range between solar and [Fe/H]=-3. LTE abundances were obtained using Kurucz...
  • Publication
    Cu, Ba and Y in FGK main-sequence stars from the HARPS sample
    It is well known that at a given [Fe/H] below solar metallicities the thick disk stars are more enhanced in their alpha -element abundances than the thin disk...
  • Publication
    Current concept for the 4m European Solar Telescope (EST) optical design
    The European Solar Telescope (EST) is a pan-european project (with 29 partners, plus 7 collaborating institutions, from 14 countries) for the conceptual design...
  • Publication
    Current concept for the 4m European Solar Telescope (EST) optical design
    The European Solar Telescope (EST) is a 4-m class solar telescope to be located in the Canary Islands which is currently in its conceptual design study. EST is...
  • Publication
    Current hot questions on the s process in AGB stars
    Asymptotic giant branch (AGB) stars are a main site of production of nuclei heavier than iron via the s process. In massive (>4 M⊙) AGB stars the operation of...