Publication type: Non-refereed

  • Publication
    Status of known T type sources towards the σ Orionis cluster
    We present the characterization of the three T type candidates (S Ori 70, S Ori 73, and S Ori J053804.65-021352.5) lying in the line of sight towards σ Orionis...
  • Publication
    Status of the Calan-Hertfordshire Extrasolar Planet Search
    In these proceedings we give a status update of the Calan-Hertfordshire Extrasolar Planet Search, an international collaboration led from Chile that aims to...
  • Publication
    Status of the design and fabrication of the GTC mirrors
    The Gran Telescopio Canarias (GTC) is a 10 m-class telescope which is under construction and will be operational at the Observatorio del Roque de Los Muchachos...
  • Publication
    Status of the EMIR mechanical system
    EMIR is the NIR multi-object imager and spectrograph for the GTC (Gran Telescopio Canarias). The instrument ADR (Advanced Design Review) was held successfully...
  • Publication
    Status of the EMIR optical system
    EMIR is a intermediate resolution near infrared (1.0 - 2.5 microns) multiobject spectrograph with image capabilities, to be mounted on the Gran Telescopio...
  • Publication
    Status of the European Solar Telescope control system
    The European Solar Telescope (EST) aims to become the most ambitious ground-based solar telescope in Europe. This paper summaries the planned architecture...
  • Publication
    Status of the GEO600 detector
    Of all the large interferometric gravitational-wave detectors, the German/British project GEO600 is the only one which uses dual recycling. During the four...
  • Publication
    Status of the OTELO project
    The OTELO project is the extragalactic survey currently under way using the tunable filters of the OSIRIS instrument at the GTC. OTELO is already providing the...
  • Publication
    Status of the physics of substellar objects
    A full understanding of the properties of substellar objects is one of the major challenges facing astrophysics. Since their discovery in 1995, we have...