• Charla
    (1) Seismology of stars: problems and prospects (2) Asteroseismic CoRoT targets and the ground-based follow-up observations (3) Classical novae and cataclysmic variables: a modern perspective
    The asteroseismic window of the CoRoT satellite mission aims at the monitoring of several types of pulsators along the Main Sequence. To optimise the science...
  • Publicación
    1000 cataclysmic variables from the Catalina Real-time Transient Survey
    Over six years of operation, the Catalina Real-time Transient Survey (CRTS) has identified 1043 cataclysmic variable (CV) candidates - the largest sample of CVs...
  • Publicación
    1RXS J062518.2+733433: A new intermediate polar
    We report the identification of the cataclysmic variable 1RXS J062518.2+733433 as an intermediate polar. The orbital period of the system is determined to be...
  • Publicación
    A 15.7-minAM CVn binary discovered in K2
    We present the discovery of SDSS J135154.46-064309.0, a short-period variable observed using 30-mincadence photometry in K2 Campaign 6. Follow-up spectroscopy...
  • Publicación
    A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole
    Two years after its outburst in 1989, the William Herschel Telescope has been used to find absorption features in V404 Cyg characteristic of a late G or early K...
  • Publicación
    A catalogue of orbital periods of cataclysmic variables and candidates from TESS observations
    We present a systematic analysis of 2544 cataclysmic variable systems and related candidates observed by the Transiting Exoplanet Survey Satellite (TESS), with...
  • Publicación
    A feasibility study on the photometric detection of quiescent black hole X-ray binaries
    We investigate the feasibility of detecting quiescent black hole X-ray binaries using optical photometric techniques. To test this, we employ a combination of r...
  • Publicación
    A FWHM–K2 Correlation in Black Hole Transients
    We compare {{{H}}}α emission profiles of 12 dynamically confirmed black holes (BHs) and 2 neutron star X-ray transients (SXTs) in quiescence with those of a...
  • Publicación
    A Hα metric for identifying dormant black holes in X-ray transients
    Dormant black holes in X-ray transients can be identified by the presence of broad Hα emission lines from quiescent accretion discs. Unfortunately, short-period...