Publication type: Refereed

  • Publication
    The Asteroseismic Potential of Kepler: First Results for Solar-Type Stars
    We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5 days of...
  • Publication
    The ASTRI Mini-Array of Cherenkov telescopes at the Observatorio del Teide
    The ASTRI Mini-Array (MA) is an INAF project to build and operate a facility to study astronomical sources emitting at very high-energy in the TeV spectral band...
  • Publication
    The astronomy and astrology of Isidore of Seville.
    Not Available
  • Publication
    The AT-LESS CO(1-0) survey of submillimetre galaxies in the Extended Chandra Deep Field South: First results on cold molecular gas in galaxies at z ˜ 2
    We present the first results from our ongoing Australia Telescope Compact Array survey of 12CO(1-0) in Atacama Large Millimeter Array (ALMA)-identified...
  • Publication
    The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters
    We present a catalog of 4195 optically confirmed Sunyaev–Zel’dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio >4 in 13,211 deg 2 of sky...
  • Publication
    The Atacama Large Aperture Submillimeter Telescope (AtLAST)
    Overview of the science cases for, and technologies required for a new single dish sub-mm telescope. AtLAST is envisioned as a 50m diameter single dish with a...
  • Publication
    The ATLAS3D project - XXII. Low-efficiency star formation in early-type galaxies: hydrodynamic models and observations
    We study the global efficiency of star formation in high-resolution hydrodynamical simulations of gas discs embedded in isolated early-type and spiral galaxies...
  • Publication
    The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve
    Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperatures that are comparable to those of the coldest stars. These...
  • Publication
    The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution
    We observed two transits of the iconic gas giant HD 209458b between 380 and 780 nm, using the high-resolution ESPRESSO spectrograph. The derived planetary...