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About

Matthew Cornachione is an astronomer specializing in exoplanet detection and characterization, with a particular focus on ground-based follow-up facilities. His primary research involves the confirmation and mass measurement of transiting exoplanets discovered by space missions like TESS, especially those orbiting bright stars. Cornachione’s most notable contribution is his lead role in the design, commissioning, and first photometric results of the MINERVA-Australis telescope array, detailed in his 2019 paper (21 citations). This facility is one of the few in the Southern Hemisphere dedicated exclusively to the follow-up and characterization of TESS planet candidates, filling a critical niche in exoplanet science. By enabling precise radial velocity measurements and photometric monitoring, MINERVA-Australis has become instrumental in validating new worlds and measuring their masses. Cornachione’s work bridges the gap between space-based discovery and ground-based confirmation, directly advancing our understanding of planetary systems around nearby, bright stars—a key step toward future atmospheric characterization.