In June 2023, NANOGrav (the North American Nanohertz Observatory for Gravitational Waves), among other PTAs, provided very strong evidence for detection of the nanohertz gravitational wave background. This background is theorized to originate from a symphony of supermassive binary black hole mergers. With improved timing precision and more pulsars, we will be able to resolve the signals of individual mergers.

The interstellar medium (ISM), which is the turbulent gas and dust in space, induces propagation effects for pulsar signals. These effects limit the precision of pulsar timing, and improved understanding is necessary. As a NANOGrav Junior Member, the focus of my current research is scattering, temporal broadening of a pulsar signal due to diffraction through variations in electron density in the ISM. Through analysis of scattering, we improve pulsar timing and better understand turbulence in the ISM along the line of sight. We have recently had a paper accepted for publication with the Astrophysical Journal on this work found here.

I spent summer 2024 at Caltech, conducting a research project focused on the circumgalactic medium under the mentorship of Professor Vikram Ravi entitled "Tracing the Milky Way Circum-Galactic Medium With Optical Spectroscopy".

Since January of 2025, I have also been working with Professor Eanna Flanagan at Cornell on theoretical research related to gravitational waves. I will be working on a senior thesis focused on the potential for detection of gravitational wave memory with astromety. I am spending summer of 2025 working on this project.

Presentations and Publications