Publication type: Non-refereed

  • Publication
    The optical counterparts of Accreting Millisecond X-Ray Pulsars during quiescence
    Using data obtained with the ESO-Very Large Telescope, we have performed a deep optical and NIR photometric study of the fields of three Accreting Millisecond X...
  • Publication
    The Optical Properties of the Host Galaxies of FR I and FR II Radio Sources
    The two Fanaroff & Riley classes of radio galaxies are defined by radio morphology, and the distinction may arise from a combination of environmental conditions...
  • Publication
    The optical variability of 3C 345.
    The publication by Lloyd (1984) of new and revised data for a sample of active nuclei brought the number of published observations of 3C 345 up to over 900...
  • Publication
    The optical variability of the magic blazar PKS 1222+216
    Not Available
  • Publication
    The optical, infrared and radio light curve of OJ 287 during winter 1993 - 94.
    The light curves of OJ 287 at UBVRIJHK, 22 and 37 GHz are presented for the 1993/94 observing campaign. Despite the considerable optical and infrared activity...
  • Publication
    The OPTICON A2IM Cookbook: an introduction to additive manufacture for astronomy
    Additive manufacture (AM), also known as 3D printing, builds an object, layer-by-layer, from a digital design file. The primary advantage of the layer-by-layer...
  • Publication
    The opto-mechanical design of HARMONI: a first light integral field spectrograph for the E-ELT
    HARMONI is a visible and near-IR integral field spectrograph, providing the E-ELT's spectroscopic capability at first light. It obtains simultaneous spectra of...
  • Publication
    The orbital period of the Galactic Z source SCO X-2
    Not Available
  • Publication
    The orbital phases and secondary transit of Kepler-10b - A physical interpretation based on the Lava-ocean planet model -
    In this presentation, we apply the Lava-ocean model that has been proposed for planets of the class of CoRoT-7b, i.e. rocky planets at a few stellar radii from...