Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Astro and Planetary Science, and Astrophysics and Star Formation Studies.
JWST Directly Images Giant Planet Candidates Around Two Metal-polluted White Dwarf Stars
A MIRI Search for Planets and Dust around WD 2149+021
Three’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets
TERRESTRIAL PLANET OCCURRENCE RATES FOR THE<i>KEPLER</i>GK DWARF SAMPLE
PLANETARY CANDIDATES OBSERVED BY <i>KEPLER</i> . VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS)
PLANETARY CANDIDATES OBSERVED BY <i>KEPLER</i> . V. PLANET SAMPLE FROM Q1–Q12 (36 MONTHS)
VALIDATION OF<i>KEPLER</i>'S MULTIPLE PLANET CANDIDATES. III. LIGHT CURVE ANALYSIS AND ANNOUNCEMENT OF HUNDREDS OF NEW MULTI-PLANET SYSTEMS
MASSES, RADII, AND ORBITS OF SMALL <i>KEPLER</i> PLANETS: THE TRANSITION FROM GASEOUS TO ROCKY PLANETS
PLANETARY CANDIDATES OBSERVED BY <i>KEPLER</i> IV: PLANET SAMPLE FROM Q1-Q8 (22 MONTHS)
PLANETARY CANDIDATES OBSERVED BY <i>KEPLER</i> . III. ANALYSIS OF THE FIRST 16 MONTHS OF DATA
FUNDAMENTAL PROPERTIES OF<i>KEPLER</i>PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY
Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone
A sub-Mercury-sized exoplanet
Alignment of the stellar spin with the orbits of a three-planet system
PHOTOMETRICALLY DERIVED MASSES AND RADII OF THE PLANET AND STAR IN THE TrES-2 SYSTEM
Three ways to solve the orbit of KIC 11 558 725: a 10-day beaming sdB+WD binary with a pulsating subdwarf
Seismic evidence for non-synchronization in two close sdb+dM binaries from Kepler photometry