Tipo de publicación: Con árbitro

  • Publicación
    Characterization of seven transiting systems, including four warm Jupiters from SOPHIE and TESS
    While several thousand exoplanets are now confirmed, the number of known transiting warm Jupiters (10 d < period < 200 d) remains relatively small. These...
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    Characterization of starspots on a young M-dwarf K2-25: multiband observations of stellar photometric variability and planetary transits
    Detailed atmospheric characterization of exoplanets by transmission spectroscopy requires careful consideration of stellar surface inhomogeneities induced by...
  • Publicación
    Characterization of telescope polarization properties across the visible and near-infrared spectrum. Case study: the Dunn Solar Telescope
    Accurate astrophysical polarimetry requires a proper characterization of the polarization properties of the telescope and instrumentation employed to obtain the...
  • Publicación
    Characterization of the Ejecta from the NASA/DART Impact on Dimorphos: Observations and Monte Carlo Models
    The NASA Double Asteroid Redirection Test (DART) spacecraft successfully crashed on Dimorphos, the secondary component of the binary (65803) Didymos system...
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    Characterization of the HD 108236 system with CHEOPS and TESS Confirmation of a fifth transiting planet
    Context. The HD 108236 system was first announced with the detection of four small planets based on TESS data. Shortly after, the transit of an additional...
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    Characterization of the HD 17156 planetary system
    Aims: We present data to improve the known parameters of the HD 17156 system (peculiar due to the eccentricity and long orbital period of its transiting planet)...
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    Characterization of the June epsilon Ophiuchids meteoroid stream and the comet 300P/Catalina
    Aims: Prior to 2019, the June epsilon Ophiuchids (JEO) were known as a minor unconfirmed meteor shower with activity that was considered typically moderate for...
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    Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date
    Context. An accurate characterization of the known exoplanet population is key to understanding the origin and evolution of planetary systems. Determining true...
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    Characterization of the known T-type dwarfs towards the σ Orionis cluster
    Aims: The detailed study of T-type candidate members of the young σ Orionis cluster (~3 Myr, ~352 pc, solar metallicity) is fundamental to properly assess the...