Publication type: Refereed

  • Publication
    The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type spiral
    Understanding star formation in galaxies requires resolving the physical scale on which star formation often occurs: the scale of star clusters. We present a...
  • Publication
    The PAU Survey and Euclid: Improving broadband photometric redshifts with multi-task learning
    Current and future imaging surveys require photometric redshifts (photo-zs) to be estimated for millions of galaxies. Improving the photo-z quality is a major...
  • Publication
    The PAU survey: classifying low-z SEDs using Machine Learning clustering
    We present an application of unsupervised Machine Learning clustering to the PAU survey of galaxy spectral energy distribution (SED) within the COSMOS field...
  • Publication
    The PAU survey: Enhancing photometric redshift estimation using DEEPz
    We present photometric redshifts for 1 341 559 galaxies from the Physics of the Accelerating Universe Survey (PAUS) over 50.38 deg 2 of sky to i AB = 23...
  • Publication
    The PAU Survey: Galaxy stellar population properties estimates with narrowband data
    A newfound interest has been seen in narrowband galaxy surveys as a promising method for achieving the necessary accuracy on the photometric redshift estimate...
  • Publication
    The PAU survey: photometric redshift estimation in deep wide fields
    We present photometric redshifts (photo-z) for the deep wide fields of the Physics of the Accelerating Universe Survey (PAUS), covering an area of $\sim$50 deg...
  • Publication
    The PDS 110 observing campaign - photometric and spectroscopic observations reveal eclipses are aperiodic
    PDS 110 is a young disc-hosting star in the Orion OB1A association. Two dimming events of similar depth and duration were seen in 2008 (WASP) and 2011 (KELT)...
  • Publication
    The peculiar Balmer line profiles of OQ 208
    Spectrophotometric observations of OQ 208 over the time period between March 1985 and February 1991 are presented. It is found that the H-beta flux varies...
  • Publication
    The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 - Li enhancement
    Using high-resolution optical spectroscopy we determine the chemical abundance of the secondary star in the binary millisecond pulsar PSR J1023+0038. We measure...