Publication type: Refereed

  • Publication
    Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076
    Context. TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young (340 ± 80 Myr) K-type star. Although a validated...
  • Publication
    Under the same sky with Amanar
    The support of the international astronomical community to the 2030 Agenda for Sustainable Development is fundamental to advance the rights and needs of the...
  • Publication
    Understanding 26Al Emission from Cygnus
    The COMPTEL observations of the galactic 1.809 MeV emission attributed to the radioactive decay of 26Al have confirmed the diffuse nature of this interstellar...
  • Publication
    Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
    We illustrate the extraordinary discovery potential for extragalactic astrophysics of a far-infrared/submillimetre (far-IR/submm) all-sky spectroscopic survey...
  • Publication
    Understanding internetwork magnetic fields as determined from visible and infrared spectral lines
    We present numerical experiments aimed at understanding why near-infrared observations systematically deliver weak magnetic fields in the internetwork, whereas...
  • Publication
    Understanding sudden changes in cloud amount: The Southern Annular Mode and South American weather fluctuations
    This work investigates the cause and effects of extreme changes in synoptic-scale cloud cover operating at daily timescales using a variety of satellite-based...
  • Publication
    Understanding the Angular Momentum Evolution of T Tauri and Herbig Ae/Be Stars
    We investigate a sample of six Herbig Ae/Be stars belonging to the Orion OB1 association, as well as 73 low-mass objects, members of the σ Orionis cluster, in...
  • Publication
    Understanding the Cosmic Mass Function High-Mass Behavior
    We claim that the discrepancy found between the theoretical predictions for the cosmic mass function and those found in numerical simulations is due to the fact...
  • Publication
    Understanding the evolution and dust formation of carbon stars in the Large Magellanic Cloud via the JWST
    Context. Carbon stars have been, and still are, extensively studied. Given their complex internal structure and their peculiar chemical composition, they are...