Publication type: Non-refereed

  • Publication
    Detailed Magnetic Field Morphology of the Vela C Molecular Cloud from the BLASTPol 2012 flight
    In order to understand the role of magnetic fields in the process of star formation, we require detailed observations of field morphology on scales ranging from...
  • Publication
    Detailed processes accompanying the decay of an active region
    The decay of a small solar active region is studied with high-resolution magnetograms. The reduction process made it possible to match intensity and magnetic...
  • Publication
    Detailed processes accompanying the decay of an active region.
    High resolution (better than 1arcsec) magnetograms obtained at the Sacramento Peak Vacuum Tower Telescope were used to study the decay of a small active region...
  • Publication
    Detailed Stellar Population Analysis of Galaxy Clusters at Increasing Redshift: A Constrain for Their Evolution
    This contribution describes a project of a detailed stellar population analysis for different clusters of galaxies with increasing redshift. The selected...
  • Publication
    Detailed study of 200-mbar wind speed at the Canary Islands
    We present a comprehensive and reliable statistics of 200 mbar wind speeds at the Canary Islands based on long term climate diagnostics archive data and balloon...
  • Publication
    Detectability of Jupiter-to-Brown-Dwarf-Mass Companions Around Small Eclipsing Binary Systems
    Not Available
  • Publication
    Detecting individual gravity modes in the Sun: Chimera or reality?
    Over the past 15 years, our knowledge of the interior of the Sun has tremendously progressed by the use of helioseismic measurements. However, to go further in...
  • Publication
    Detection and Characterization of Galaxy Systems at Intermediate Redshift.
    This thesis is divided into two very related parts. In the first part we implement and apply a galaxy cluster detection method, based on multiband observations...
  • Publication
    Detection and measurement of expanding ionized shells around young star clusters
    We present a new method (BUBBLY) for detecting expanding components of ionized gas using integral field spectroscopy, showing its capabilities not only in...