Publication type: Non-refereed

  • Publication
    Final analysis of ELAIS 15-{mu}m (Vaccari+, 2005)
    We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-{mu}m observations, carried out with the ISO Camera...
  • Publication
    Final assembly, metrology, and testing of the WEAVE fibre positioner
    WEAVE is the new wide-field spectroscopy facility for the prime focus of the William Herschel Telescope at La Palma, Spain. Its fibre positioner is essential...
  • Publication
    Final design and progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope
    We present the Final Design of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), together with a status update on the...
  • Publication
    Final design of the GTC laser guide star wavefront sensor
    The Laser Guide Star Facility (LGSF) of GTC will generate a laser guide star (LGS) in the high atmosphere for the GTC Adaptive Optics System (GTCAO) to measure...
  • Publication
    Final optical design for the WEAVE two-degree prime focus corrector
    WEAVE is the next-generation wide-field optical spectroscopy facility for the William Herschel Telescope (WHT) in La Palma, Canary Islands, Spain. We present...
  • Publication
    Finding AGN Host Galaxies with HST, and the Joint Analysis with Ground Based Images.
    Understanding the connection between normally evolving galaxies and those with extreme nuclear activity, the so-called Active Galactic Nuclei, is a fundamental...
  • Publication
    Finding extra-solar planets in the presence of stellar jitter
    Not Available
  • Publication
    Finding the compositional diversity of the Solar System
    Asteroids can be defined as objects that do not have an atmosphere, are smaller than the planets and orbit the Sun. But, what is most important, asteroids are...
  • Publication
    Finding the limits of galaxies up to z = 1
    The superb depth of present ultradeep observations and next generation synoptic surveys allow us to reach sudden decrements of the galaxy surface brightness in...