Publication type: Non-refereed

  • Publication
    Dissecting the Accretion Environments of X-ray Binaries with High Speed Coordinated Optical and X-ray Timing Observations
    We are uncovering significant optical variability in low/hard state observations of several X-ray binaries on the fastest time-scales of just tens of...
  • Publication
    Dissecting the Large Magellanic Cloud: a high spatial resolution map of its star formation history
    Detailed studies of nearby Local Group galaxies offer an unique window to understanding galaxy formation and evolution. The analysis of Colour-Magnitude...
  • Publication
    Distance determination to PNe using the extinction-distance method
    We present individual distances to three PNe: NGC 6537, NGC 6781 and NGC 7027, determined by the extinction-distance method. These objects are part of a larger...
  • Publication
    Distance of 72 Galactic globular clusters (Recio-Blanco+, 2005)
    We present distance modulus and reddening determinations for 72 Galactic globular clusters from the homogeneous photometric database of Piotto et al. (2002, cat...
  • Publication
    Distance of 72 Galactic globular clusters (Recio-Blanco+, 2005)
    Apparent ZAHB F555W magnitude for 72 Galactic globular clusters, corresponding distance modulus in F555W, the reddening in flight system E(F439W-F555W) , the...
  • Publication
    Distance to W UMa stars
    In order to develop a reliable method of distance determination of W UMa-type stars, a catalogue of light curve solutions of 159 systems has been compiled. The...
  • Publication
    Distances to galaxies from the brightest stars in the Universe
    Not Available
  • Publication
    Distances to globular cluster-rich UDGs: The case of NGC1052-DF2
    Some ultra-diffuse galaxies (UDGs) are known to host very large globular cluster (GC) systems, clearly exceeding the expectations for galaxies with such low...
  • Publication
    Distances to Planetary Nebulae: A Key to Galactic Structure and Evolution
    The knowledge of accurate distances to Planetary Nebulae (PNe) is necesary in order to improve the determination of some physical quantities such as the nebular...