Publications

  • Obliquity measurement and atmospheric characterisation of the WASP-74 planetary system

    We present new transit observations of the hot Jupiter WASP-74 b (Teq ~ 1860 K) using the high-resolution spectrograph HARPS-N and the multi-colour simultaneous imager MuSCAT2. We refined the orbital properties of the planet and its host star and measured its obliquity for the first time. The measured sky-projected angle between the stellar spin

    Luque, R. et al.

    Advertised on:

    10
    2020
  • The Gaia-ESO Survey: A new diagnostic for accretion and outflow activity in the young cluster NGC 2264

    Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by taking advantage of the FLAMES data in the context of the Gaia-ESO Survey. In fact, the analysis of the Hα emission line profile can provide us with information about the accretion and ejection activity of young stars. However, a strong nebular emission

    Bonito, R. et al.

    Advertised on:

    10
    2020