Publication type: Non-refereed

  • Publication
    Development of the camera for the large size telescopes of the Cherenkov Telescope Array
    The Large Size Telescopes, LSTs, located at the center of the Cherenkov Telescope Array, CTA, will be sensitive for low energy gamma-rays. The camera on the LST...
  • Publication
    Development status of the telescope for the Ingenio/SEOSAT mission primary payload
    Ingenio/SEOSAT is the flagship mission for the Spanish Space Plan 2007-2011, as is currently under development by a Spanish industrial consortium in the...
  • Publication
    Developments in fiber-positioning technology for the WEAVE instrument at the William Herschel Telescope
    WEAVE is the next-generation wide-field optical spectroscopy facility for the William Herschel Telescope (WHT) on La Palma in the Canary Islands, Spain. It is a...
  • Publication
    DG Leo uvby differential photometry (Lampens+, 2005)
    The first table (dataset1) contains 1590 data points collected with 1.5m telescopes equipped with conventional photometers at the observatories of San Pedro...
  • Publication
    Diagnostic diagrams of H 0 regions in the Local Group
    We have studied here for the first time the use of the log(H 0/[N 0]), log (H 0/[S 0]) diagnostic diagram for determining the metallicities and ionization...
  • Publication
    Diagnostic methods based on scattering polarization and the joint action of the Hanle and Zeeman effects
    Polarized light provides the most reliable source of information at our disposal for diagnosing the physical properties of astrophysical plasmas, including the...
  • Publication
    Diagnostic of prominence magnetic fields
    An updated review on theoretical research on the role of magnetic fields in prominences is presented. It is concluded that the theory of the Hanle effect has...
  • Publication
    Diagnostic of the solar atmosphere using iron lines.
    Not Available
  • Publication
    Diagnostics for spectropolarimetry and magnetography
    An assessment on the capabilities of modern spectropolarimeters and magnetographs is in order since most of our astrophysical results rely upon the accuracy of...