Publication type: Non-refereed

  • Publication
    ALIOLI: Adaptive and Lucky Imaging Optics Lightweight Instrument
    As a consequence of the evolution in the design and of the modularity of its components, AOLI for the William Herschel Telescope (WHT 4.2m) is much smaller and...
  • Publication
    ALIOLI: presentation and first steps
    Adaptive optics (AO) systems correct atmospheric turbulence in real time and they are normally used in large and medium telescopes but not in modest telescopes...
  • Publication
    ALISIO-1 mission: bridging space and Earth with next-generation CubeSat for optical communications and environmental monitoring
    ALISIO-1, the first satellite owned and led by the Instituto de Astrofısica de Canarias (IAC), represents a significant milestone in the space exploration of...
  • Publication
    All Sky Survey For Planet Detection By Transits
    PASS, the Permanent All Sky Survey is a project to survey the entire visible sky for the presence of transits by extrasolar planets. The instrument would...
  • Publication
    All-Sky Cameras Detection and Telescope Follow-Up of the 17P/Holmes Outburst
    Cometary outbursts are not completely understood. We have performed a continuous coverage of the recent 17P/Holmes outburst in order to learn more about the...
  • Publication
    ALMA correlator computer systems
    We present a design for the computer systems which control, configure, and monitor the Atacama Large Millimeter Array (ALMA) correlator and process its output...
  • Publication
    ALMA spectrum of the extreme OH/IR star OH 26.5+0.6
    We present ALMA band 7 data of the extreme OH/IR star, OH 26.5+0.6. In addition to lines of CO and its isotopologues, the circumstellar envelope also exhibits a...
  • Publication
    Along the path towards extremely precise radial velocity measurements
    In the last six years, thanks to the very high radial velocity precision of the HARPS spectrograph, it was possible to detect 21 out of the 30 super-Earth...
  • Publication
    Alpha Per faint stars photometry (Barrado y Navascues+, 2002)
    We obtained deep optical imaging of the Alpha Per open cluster using the KPNO 4-m CCD mosaic camera, MOSA, on November 19-22 1998. All of the images were...