Publication type: Non-refereed

  • Publication
    Optical-component-only adaptive optics improved setup
    This paper introduces a new technique for performing binary adaptive optics using optical components only, without the help of any electronic, or optoelectronic...
  • Publication
    Optical-near infrared photometry of the Galactic globular cluster NGC 6441 .
    We present optical- near infrared photometry of the peculiar Galactic globular cluster NGC 6441. By using the K-band Period-Luminosity-Metallicity (PLZK) of its...
  • Publication
    Optical/IR flux fading rapidly in GX 339-4: OIR jet quenching
    The transient black hole candidate GX 339-4 is currently softening in X-ray, making a transition out of the hard state (ATel #2545). We are monitoring the...
  • Publication
    Optical/near-IR observations of SGR 1900+14 during the May-June and Aug-Sep 1998 active periods
    We present the results of optical/IR observations obtained in the period June-October 1998. Images in the Gunn-z band were serendipitously taken just 3 days...
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    Optical/NIR observations of GRB001109.
    Not Available
  • Publication
    Optics of the instrument Elmer for the GTC 10-m telescope
    Elmer is a visible imager and spectrograph for the Gran Telescopio Canarias, which has been designed in-house. The major features and some of the analysis done...
  • Publication
    Optimisation of the WEAVE target assignment algorithm
    WEAVE is the new wide-field spectroscopic facility for the prime focus of the William Herschel Telescope in La Palma, Spain. Its fibre positioner is essential...
  • Publication
    Optimising rapid autonomous transient classifications with the New Robotic Telescope
    The New Robotic Telescope (NRT), the 4-metre, next-generation Liverpool Telescope (LT), will be located on La Palma, Canary Islands. The design and development...
  • Publication
    Optimizing TESS short cadence aperture for Asteroseismology of solar-like stars
    Thanks to missions such as CoRoT and Kepler/K2, asteroseismology has demonstrated that it is a powerful tool to determine precise stellar parameters. Now, with...