PhD student in the Astrophotonics Technology Lab at the University of California, Los Angeles (UCLA).
My research focuses on the simulation and development of an H-band photonic nulling beam combiner for the CHARA Array.
The Astrophotonics Technology (APT) Lab at UCLA advances astronomy through integrated photonics.
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Long baseline interferometry is a technique used to achieve high angular resolution observations by combining the light from multiple telescopes.
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Long baseline nulling interferometry is a powerful technique for characterizing exoplanets by measuring their properties and atmospheres.
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S. Morrison et al., Proceedings of SPIE Astronomical Telescopes and Instrumentation, upcoming
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S. Morrison et al., Proceedings of SPIE 13627, Techniques and Instrumentation for Detection of Exoplanets XII (2025)
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