Publication type: Refereed

  • 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...
  • Publication
    Asteroseismology and interferometry
    Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the first...
  • Publication
    Asteroseismology and Spectropolarimetry of the Exoplanet Host Star λ Serpentis
    The bright star λ Ser hosts a hot Neptune with a minimum mass of 13.6 M ⊕ and a 15.5 day orbit. It also appears to be a solar analog, with a mean rotation...
  • Publication
    Asteroseismology from multi-month Kepler photometry: the evolved Sun-like stars KIC 10273246 and KIC 10920273
    Context. The evolved main-sequence Sun-like stars KIC 10273246 (F-type) and KIC 10920273 (G-type) were observed with the NASA Kepler satellite for approximately...
  • Publication
    Asteroseismology of 19 low-luminosity red giant stars from Kepler
    Context. Frequencies of acoustic and mixed modes in red giant stars are now determined with high precision thanks to the long continuous observations provided...
  • Publication
    Asteroseismology of iota Draconis and Discovery of an Additional Long-period Companion
    Giant stars as known exoplanet hosts are relatively rare due to the potential challenges in acquiring precision radial velocities and the small predicted...
  • Publication
    Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-d binary system
    The candidate SX Phe star KIC 11754974 shows a remarkably high number of combination frequencies in the Fourier amplitude spectrum: 123 of the 166 frequencies...