Publication type: Refereed

  • Publication
    WeCAPP - Wendelstein Calar Alto pixellensing project I. Tracing dark and bright matter in M 31
    We present WeCAPP, a long term monitoring project searching for microlensing events towards M 31. Since 1997 the bulge of M 31 was monitored in two different...
  • Publication
    Weighing stars from birth to death: mass determination methods across the HRD
    The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar...
  • Publication
    Welcome to the Twilight Zone: The Mid-infrared Properties of Post-starburst Galaxies
    We investigate the optical and Wide-field Survey Explorer (WISE) colors of “E+A” identified post-starburst galaxies, including a deep analysis of 190 post...
  • Publication
    Westerlund 1 under the light of Gaia EDR3: Distance, isolation, extent, and a hidden population
    Context. The young massive cluster Westerlund 1 offers the promise of a grand laboratory for the study of high-mass star evolution, but its basic parameters are...
  • Publication
    WET Observations of GD 358 in 2000
    We report on the 323 hours of nearly uninterrupted time series photometric observations of the DBV star GD 358 acquired with the Whole Earth Telescope (WET)...
  • Publication
    WHaD diagram: Classifying the ionizing source with one single emission line
    Context. The usual approach to classify the ionizing source using optical spectroscopy is based on the use of diagnostic diagrams that compare the relative...
  • Publication
    What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24?
    Characterizing the structural properties of galaxies in high-redshift protoclusters is key to our understanding of the environmental effects on galaxy evolution...
  • Publication
    What do Simulations Predict for the Galaxy Stellar Mass Function and its Evolution in Different Environments?
    We present a comparison between the observed galaxy stellar mass function and the one predicted from the De Lucia & Blaizot semi-analytic model applied to the...
  • Publication
    What drives the variance of galaxy spectra?
    We present a study aimed at understanding the physical phenomena underlying the formation and evolution of galaxies following a data-driven analysis of...