Dr. Gregg Hallinan photo
Principal Investigator
California Institute of Technology

1200 East California Boulevard
Division of Physics, Mathematics and Astronomy
Mail Code 249-17
Pasadena, CA 91125

The study of magnetic activity of stars, brown dwarfs and exoplanets with particular focus on the search for magnetospheric radio emissions from exoplanets from ground and space. The detection and classification of radio transient sources at MHz and GHz frequencies. Characterization of the size distribution of the Kuiper belt. PI of the OVRO-LWA low frequency all-sky imaging array, the Deep Synoptic Array (DSA) to detect and localize FRBs and the CHIMERA high-speed optical photometer.

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