Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies, and Astro and Planetary Science.
Expanding the frontiers of cool-dwarf asteroseismology with ESPRESSO
Low-amplitude Solar-like Oscillations in the K5 V Star ϵ Indi A
A 20 Second Cadence View of Solar-type Stars and Their Planets with TESS: Asteroseismology of Solar Analogs and a Recharacterization of π Men c
Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi
Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite
A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by <i>TESS</i>
Repository of the Academy's Library (Library of the Hungarian Academy of Sciences) 2019cited by 85position: middle
An asteroseismic view of the radius valley: stripped cores, not born rocky
First Results from the Hertzsprung SONG Telescope: Asteroseismology of the G5 Subgiant Star μ Herculis*
Hot super-Earths stripped by their host stars
A 1.9 EARTH RADIUS ROCKY PLANET AND THE DISCOVERY OF A NON-TRANSITING PLANET IN THE KEPLER-20 SYSTEM*
THE KEPLER-454 SYSTEM: A SMALL, NOT-ROCKY INNER PLANET, A JOVIAN WORLD, AND A DISTANT COMPANION
Ages and fundamental properties of<i>Kepler</i>exoplanet host stars from asteroseismology
AN ANCIENT EXTRASOLAR SYSTEM WITH FIVE SUB-EARTH-SIZE PLANETS
Oscillation frequencies for 35<i>Kepler</i>solar-type planet-hosting stars using Bayesian techniques and machine learning
KEPLER-432: A RED GIANT INTERACTING WITH ONE OF ITS TWO LONG-PERIOD GIANT PLANETS
MASSES, RADII, AND ORBITS OF SMALL <i>KEPLER</i> PLANETS: THE TRANSITION FROM GASEOUS TO ROCKY PLANETS
Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7
LIMITS ON SURFACE GRAVITIES OF<i>KEPLER</i>PLANET-CANDIDATE HOST STARS FROM NON-DETECTION OF SOLAR-LIKE OSCILLATIONS
FUNDAMENTAL PROPERTIES OF<i>KEPLER</i>PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
Stellar Spin-Orbit Misalignment in a Multiplanet System
A sub-Mercury-sized exoplanet
ASTEROSEISMIC DETERMINATION OF OBLIQUITIES OF THE EXOPLANET SYSTEMS KEPLER-50 AND KEPLER-65
Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities
Kepler-22b: A 2.4 EARTH-RADIUS PLANET IN THE HABITABLE ZONE OF A SUN-LIKE STAR