Astrophysical: Methods

  • Publication
    Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b
    The spectral signatures of optical absorbers, when combined with those of infrared molecules, play a critical role in constraining the cloud properties of...
  • Publication
    Detection of satellite remnants in the Galactic halo with Gaia- III. Detection limits for ultrafaint dwarf galaxies
    We present a method to identify ultrafaint dwarf galaxies (UFDGs) candidates in the halo of the Milky Way using the future Gaia catalogue and we explore its...
  • Publication
    Detection of sodium in the atmosphere of WASP-69b
    Context. Transit spectroscopy is one of the most commonly used methods to characterize exoplanets' atmospheres. From the ground, these observations are very...
  • Publication
    Detection of the Effect of Cosmological Large-Scale Structure on the Orientation of Galaxies
    Galaxies are not distributed randomly throughout space but are instead arranged in an intricate ``cosmic web'' of filaments and walls surrounding bubble-like...
  • Publication
    Detections of solar-like oscillations in dwarfs and subgiants with Kepler DR25 short-cadence data
    During the survey phase of the Kepler mission, several thousand stars were observed in short cadence, allowing for the detection of solar-like oscillations in...
  • Publication
    Determination of the cross-field density structuring in coronal waveguides using the damping of transverse waves
    Context. Time and spatial damping of transverse magnetohydrodynamic (MHD) kink oscillations is a source of information on the cross-field variation of the...
  • Publication
    Determination of the spectroscopic stellar parameters for 257 field giant stars★
    The study of stellar parameters of planet-hosting stars, such as metallicity and chemical abundances, help us to understand the theory of planet formation and...
  • Publication
    Determination of Transverse Density Structuring from Propagating Magnetohydrodynamic Waves in the Solar Atmosphere
    We present a Bayesian seismology inversion technique for propagating magnetohydrodynamic transverse waves observed in coronal waveguides. The technique uses...
  • Publication
    Determining global parameters of the oscillations of solar-like stars
    Context. Helioseismology has enabled us to better understand the solar interior, while also allowing us to better constrain solar models. But now is a...