Publication type: Refereed

  • Publication
    Asteroid Lightcurves from the MOA-II Survey: a pilot study
    The Microlensing Observations in Astrophysics (MOA-II) survey has performed high cadence, wide field observations of the Galactic Bulge from New Zealand since...
  • Publication
    Asteroid pairs: A complex picture
    We studied a sample of 93 asteroid pairs, i.e., pairs of genetically related asteroids that are on highly similar heliocentric orbits. We estimated times...
  • Publication
    Asteroid reflectance spectra from Gaia DR3: Near-UV in primitive asteroids
    Context. In the context of charge-coupled devices (CCDs), the ultraviolet (UV) region has mostly remained unexplored after the 1990s. Gaia DR3 offers the...
  • Publication
    Asteroids (65) Cybele, (107) Camilla and (121) Hermione: Infrared spectral diversity among the Cybeles
    We find a clear diversity in the 3 μm and 10 μm features of three Cybele asteroids: (107) Camilla, (121) Hermione, and (65) Cybele. (121) Hermione exhibits a...
  • Publication
    Asteroids' reflectance from Gaia DR3: Artificial reddening at near-UV wavelengths
    Context. Observational and instrumental difficulties observing small bodies below 0.5 μm make this wavelength range poorly studied compared with the visible and...
  • Publication
    Asteroseismic Diagrams from a Survey of Solar-like Oscillations with Kepler
    Photometric observations made by the NASA Kepler Mission have led to a dramatic increase in the number of main-sequence and subgiant stars with detected solar...
  • Publication
    Asteroseismic Fundamental Properties of Solar-type Stars Observed by the NASA Kepler Mission
    We use asteroseismic data obtained by the NASA Kepler mission to estimate the fundamental properties of more than 500 main-sequence and sub-giant stars. Data...
  • Publication
    Asteroseismic masses of four evolved planet-hosting stars using SONG and TESS: resolving the retired A-star mass controversy
    The study of planet occurrence as a function of stellar mass is important for a better understanding of planet formation. Estimating stellar mass, especially in...
  • Publication
    Asteroseismic masses of retired planet-hosting A-stars using SONG
    To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars...