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.
Technical description and performance of the phase II version of the Keck Planet Imager and Characterizer
Water Dissociation and Rotational Broadening in the Atmosphere of KELT-20 b from High-resolution Spectroscopy
Are These Planets or Brown Dwarfs? Broadly Solar Compositions from High-resolution Atmospheric Retrievals of ∼10–30 M <sub>Jup</sub> Companions
Validation of Elemental and Isotopic Abundances in Late-M Spectral Types with the Benchmark HIP 55507 AB System
Atmospheric Metallicity and C/O of HD 189733 b from High-resolution Spectroscopy
Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy
A Uniform Analysis of Debris Disks with the Gemini Planet Imager. I. An Empirical Search for Perturbations from Planetary Companions in Polarized Light Images
Atmospheric Characterization of the Super-Jupiter HIP 99770 b with KPIC
A uniform analysis of debris discs with the Gemini Planet Imager II: constraints on dust density distribution using empirically informed scattering phase functions
Detecting Exomoons from Radial Velocity Measurements of Self-luminous Planets: Application to Observations of HR 7672 B and Future Prospects
Keck Planet Imager and Characterizer Emission Spectroscopy of WASP-33b
A Clear View of a Cloudy Brown Dwarf Companion from High-resolution Spectroscopy
Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf
Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-resolution Data
Phase II of the Keck Planet Imager and characterizer: system-level laboratory characterization and preliminary on-sky commissioning
Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign
Characterization and performance of the upgraded NIRSPEC on the W. M. Keck Telescope