About Me

Hello! I'm Andrew, a 4th year undergrad studying Physics with a Specialization in Astrophysics at UCSD. I currently work in the UCSD OIRLAB on simulations for Keck Liger, a new imager and IFS for the Keck I telescope.

I primarily characterize the wavelength solution calibration of the IFS, working with simulations of the IFS to determine how well calibrated Liger will be in its various modes, as well as the capabilities of the Keck I calibration unit to determine if it is adequate for newer generation IFSs with higher spectral resolutions than their predecessors.

Curriculum Vitae: CV

Posters and Presentations: Posters

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Research Interests

I'm currently very interested in studying the evolution and formation of galaxies through observational astronomy. Specifically, I'm interested in studying the processes by which star-forming galaxies are quenched, especially at higher redshift (z ≳ 3). A lot of interesting research has come out with the advent of JWST that allows us to analyze much fainter galaxies at earlier epochs, and I am hoping to research how these earlier galaxies were quenched, whether by mergers, AGN feedback, virial shock heating, or some other dominant factor.

I'm also extremely interested in developing and researching the photonics to observe the galaxies I wish to study. In particular, I find research in adaptive optics to be quite fascinating, as I would love to continue working in the development of new ground-based instrumentation. New and improved adaptive optics systems like the anticipated STRATA upgrade at the Keck telescopes would significantly improve the resolving capabilities of instruments like Liger. This would allow for newer ground-based instruments to observe far fainter objects, allowing us to probe further into the universe's history, and opening up more opportunities for observations at earlier epochs.

Image Credit: ESA/Webb, NASA & CSA, G. Gozaliasl, A. Koekemoer, M. Franco, and the COSMOS-Web team

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