My research focuses on uncovering the mysteries of distant worlds by studying their atmospheres. I specialize in using infrared spectroscopic phase curves, a powerful method for exploring the three-dimensional structure of exoplanet atmospheres. Through a technique called spectral retrieval, I analyze these observations to map atmospheric properties, construct energy balance models, identify wind and cloud patterns, and reveal the chemical composition of these alien worlds.
Currently, I'm applying my expertise to study WASP-121b, an ultra-hot Jupiter, using high-quality thermal emission data collected by the James Webb Space Telescope (JWST). With JWST's cutting-edge capabilities, I aim to achieve groundbreaking insights into these planets, building on decades of earlier research.
I'm also interested in advancing how we analyze exoplanet phase curves. As part of my work, I'm benchmarking different spectral retrieval methods to identify the most effective techniques for interpreting these complex datasets. This effort is critical as we prepare for the launch of the European Space Agency's ARIEL telescope in 2029, which will usher in a new era of exoplanet exploration.
Through this research, I hope to push the boundaries of our understanding of exoplanetary atmospheres and contribute to the broader effort of uncovering what these distant worlds are truly like.