Publication type: Refereed

  • Publication
    A dearth of planetary transits in the direction of NGC 6940
    We present results of our survey for planetary transits in the field of NGC 6940. We think nearly all of our observed stars are field stars. We have obtained...
  • Publication
    A dearth of small particles in the transiting material around the white dwarf WD 1145+017
    White dwarf WD 1145+017 is orbited by several clouds of dust, possibly emanating from actively disintegrating bodies. These dust clouds reveal themselves...
  • Publication
    A dearth of young and bright massive stars in the Small Magellanic Cloud
    Context. Massive star evolution at low metallicity is closely connected to many fields in high-redshift astrophysics, but is poorly understood so far. Because...
  • Publication
    A decade of near-infrared variability in NGC4388: insights into the AGN structure
    Variability studies have proven to be a powerful diagnostic tool for understanding the physics and properties of active galactic nuclei (AGNs). They provide...
  • Publication
    A Decade of the Moderate Resolution Imaging Spectroradiometer: Is a Solar-Cloud Link Detectable?
    Not Available
  • Publication
    A DECam view of the diffuse dwarf galaxy Crater II - Variable stars
    Time series observations of a single dithered field centred on the diffuse dwarf satellite galaxy Crater II were obtained with the Dark Energy Camera (DECam) at...
  • Publication
    A DECam view of the diffuse dwarf galaxy Crater II: the colour-magnitude diagram
    We present a deep Blanco/DECam colour-magnitude diagram (CMD) for the large but very diffuse Milky Way satellite dwarf galaxy Crater II. The CMD shows only old...
  • Publication
    A deep learning approach to infer galaxy cluster masses from Planck Compton-y parameter maps
    Galaxy clusters are useful laboratories to investigate the evolution of the Universe, and accurate measurement of their total masses allows us to constrain...
  • Publication
    A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations
    Hydrodynamical simulations of galaxy formation and evolution attempt to fully model the physics that shapes galaxies. The agreement between the morphology of...