Planet occurrence in the Galaxy
How metallicity, α-abundance, kinematics, and Galactic component membership change planetary rates and architectures.
Research
I connect planetary and stellar systems to the Galactic populations they come from, using large astronomical surveys and spectroscopic datasets.
Research Themes
How metallicity, α-abundance, kinematics, and Galactic component membership change planetary rates and architectures.
Metrics for comparing full planetary systems, including the Weighted Energy Distance approach.
Empirical signatures across companion masses, orbital architectures, and host properties that constrain formation theories.
Demographics across Galactic populations, compact hierarchical triples, and tidal circularization physics.
Finding black holes, neutron stars, and white dwarfs in large astrometric and spectroscopic datasets, then using their orbital parameters to probe binary evolution and formation channels.