I am interested in the study of planets that orbit around stars other than our sun, aka exoplanets. As part of NASA’s Kepler Space Mission and the California Planet Search team, I work to characterize the size, mass, density and composition of the exoplanets discovered that are the most like the Earth. Our team accomplishes this by combining photometric measurements of stars’ brightness collected by Kepler with radial velocity measurements of individual stars collected with the Keck Telescope and HIRES spectrometer located on the top of Mauna Kea on the Big Island of Hawai’i. The overarching goal of my research is to try to find planets that most resemble the Earth in their size, composition, and distance from their host star.
I am also interested in stellar activity, specifically measured by the spectral features produced in the chromospheres of stars. By studying these features, we can improve our radial velocity measurement precision, and uncover patterns in other stars that are similar to the different stellar activity cycles that we observe in the sun. Stellar activity on timescales of days, months, and years can be used to determine the rotation period, and timescale of stellar activity cycles.
My collaborators include Andrew Howard (CalTech), Erik Petigura (UCLA), Lauren Weiss (University of Hawaii), Lea Hirsch (Stanford), and BJ Fulton (CalTEch) as well as graduate students Molly Kosiarek (UCSC), Sarah Blunt (CalTech), Ryan Rubenzahl (Caltech), Lee Rosenthal (CalTech), and Aida Behmard (CalTech). Our new collaboration to measure planet masses around host-stars identified by the TESS satellite includes collaborators across the University of California, the University of Hawaii and Kansas University.
In my work with the Berkeley SETI Research center and Breakthrough Listen and the Search for Extraterrestrial Intelligence(SETI) I work with data from the Automated Planet Finder (APF) and the Levy Spectrometer. We search the high resolution spectra for laser emission lines that could originate from beyond the Earth. Such laser signals are very narrow in wavelength, allowing for detection against the broadband energy emitted by the observed stars. Breakthrough Listen has an extensive undergraduate research program taking place both in the summer and during UCB semester.
My collaborators at BSRC include Andrew Siemion, Vishal Gajjar, Julia DeMarines Dave MacMahon, Matt Lebofsky, Daniel Czech, Dave DeBoer, Brian Lacki, Danny Price (CSIRO) and also Bryan Brzycki and Sofia Sheikh.
I am currently pursuing my PhD at the University of Southern Queensland, Australia in collaboration with Stephen Kane (UC Riverside) and Brad Carter (USQ). That work is focused on exoplanets and stellar activity.
I was born and raised under the dark skies of Butte Montana. My interest in Astronomy began when I was shown Saturn through a telescope by Lloyd Magnuson, my middle school science teacher. After meandering through interest in different sciences, I landed at the Physics and Astronomy Department at San Francisco State University in San Francisco, California. There I collected both and undergraduate and Master’s Degree working with Dr. Debra Fischer, focusing my research on exoplanet detection and stellar activity metrics. After graduation, I began with working at UC Berkeley on the Kepler Space Mission operated out of NASA Ames Research Center, where I continue the search for life in the cosmos. I live with my wife, Missy in the Mission District of San Francisco.