I am a sixth year graduate student at Harvard University. I work with Prof. Karin Öberg (CfA) and Prof. Ilse Cleeves (University of Virginia) on modeling protoplanetary disk chemistry and physics. I also work with Prof. Leslie Rogers (University of Chicago) on rocky planet interior structure modeling. I completed my undergraduate work at the California Institute of Technology in Pasadena, CA, where I worked with Prof. John Johnson and Dr. Leslie Rogers on exoplanet statistics. I have now been awarded my master's degree from Harvard and am actively working towards my PhD. I have presented my work at American Astronmical Society meetings, the Kepler Science Conference II, and the International Astronomical Union's Astrochemistry VII meeting. I plan to defend my dissertation on May 3, 2021, and I will join UChicago's geophysical sciences department in September 2021 as a 51 Pegasi b Postdoctoral Fellow.
Many existing disk models do not take into account the changing physical conditions of the disk as material accretes towards the star. We seek to develop a self-consistent disk model that couples chemistry and dynamics in an efficient way.
Ultra-short-period, rocky planets can be pulled into non-spherical shapes by the extreme gravity from their host stars. We seek to model these shapes — and the resulting transit light curves — numerically.
Simple exoplanet transit models can be enhanced by taking into account the finite integration time of observations using Fisher information matrix analysis. Errors on each parameter are amplified in a predictible way, which can aid in estimating optimal exposure times.
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