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- "/assets/img/big-imgs/JWSTDI.jpg" : "JWST image of HIP 65426 b, Credit: NASA/ESA/CSA, A. Carter (UCSC), the ERS 1386 team, and A. Pagan (STScI)"
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I am a highly motivated and independent researcher seeking to transition into industry. I aim to leverage broad expertise in space-based observational techniques, novel image processing algorithms, statistical data analysis, physical modeling, and lab experience acquired through a Ph.D. in Astronomy. I learn quickly and can apply and communicate new knowledge efficiently and effectively.
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I am a highly motivated and independent researcher who recently transitioned into the aerospace industry. I aim to leverage broad expertise in space-based observational techniques, novel image processing algorithms, statistical data analysis, physical modeling, and lab experience acquired through a Ph.D. in Astronomy. I learn quickly and can apply and communicate new knowledge efficiently and effectively.
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I am currently a postdoctoral fellow in the astronomy department at The University of Texas at Austin. My research, with Professor Adam Kraus, focuses on using a novel image analysis technique called kernel-phase interferometry to directly image brown dwarfs and extrasolar planets. This technique uses self-calibrating observables to remove errors in the wavefront of light caused by interactions within the telescope. This allows me to detect companions below the classical $$ \lambda/D $$ diffraction limit. I apply this technique to imaging from the Hubble Space Telescope and JWST to detect companions to low mass stars at separations below the classical diffraction limit.
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I was previously a postdoctoral fellow in the astronomy department at The University of Texas at Austin. My research, with Professor Adam Kraus, focused on using a novel image analysis technique called kernel-phase interferometry to directly image brown dwarfs and extrasolar planets. This technique uses self-calibrating observables to remove errors in the wavefront of light caused by interactions within the telescope. This allowed me to detect companions below the classical $$ \lambda/D $$ diffraction limit. I applied this technique to imaging from the Hubble Space Telescope and JWST to detect companions to low mass stars at separations below the classical diffraction limit.
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I recently received my Ph.D. in astronomy from The University of Texas at Austin in 2023. Previously, I received my B.A. in physics and computer science from Wesleyan University in 2014 and my M.A. in astronomy in 2015 as part of Wesleyan's 5 year combined BA/MA program.
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