More Research Details

I am a research scientist working under employment of the Bay Area Environmental Research Institute working at NASA Ames Research Center. My current research involves using state-of-the-art algorithms and applying them to speckle observations in order to find high-contrast ratio companions. These speckle imaging algorithms allow for higher contrast ratio retrieval compared standard speckle interferometric techniques. Other software currently in the works will obtain speckle images of wide-field objects (e.g., open clusters, extended objects) as current attempts show images riddled with artifacts. My other research interest lie in studying calculating stellar parameters, doing interferometric image reconstruction, and other imaging techniques.

I obtained my Doctorate in Astronomy from the Physics and Astronomy Department at Georgia State University under the advisement of Prof. Fabien Baron. With the use of the CHARA Array, I aimed to further understand the nature of rapid rotating stars. I have developed codes to model rapid rotators in Julia and compared them to reconstructed images from interferometry. In addition to having studied rapid rotators, I have also analyzed a RS CVn star (chromospherically active stars) to obtain a 3D temperature and image map of its surface. While the inital 3D imaging of the rapid rotators had a few disagreements with the theoretical models, the 3D interferometric imaging code ROTIR that I developed during my PhD has set a baseline for furture 3D imaging of spheroids and binary systems. Aside from interferometric modeling and imaging, I have also worked with Prof. Stuart Jefferies, Dr. Theo ten Brummelaar, and Prof. Fabien Baron on a project for open air beam propogation.

I did my undergraduate work at San Diego State University, and recieved my Bachelor of Science in Astronomy and minor in Mathematics. At SDSU, I worked with Prof. Eric Sandquist and studied eclipsing binaries in the open cluster M 37. After obtaining my B.S., I worked with Prof. Ian Crossfield (as part of the CAMPARE program) and calculated stellar and planetary parameters for K2 systems of interest. This work required spectroscopic observations that we obtained at La Silla Observatory in Chile.

xkcd interferometry