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About

Tyson Hare is a leading astronomical instrumentation scientist whose work is shaping the next generation of giant telescopes. His primary research focus is the development of cutting-edge spectrographs and imagers, with major contributions to the Giant Magellan Telescope (GMT) and the Magellan Telescopes. Hare played a pivotal role in the GMT project, where his work on instrumentation progress—documented in a 2016 paper with 14 citations—helped advance the 24-meter telescope’s suite of tools, including the GCLEF high-resolution optical spectrograph. He also led the Magellan Infrared Multi-object Spectrograph (MIRMOS) project, a near-infrared instrument designed for frontier extragalactic science, as detailed in a 2020 paper with 7 citations. Hare’s impact extends beyond citations; his efforts have enabled precision radial velocity measurements and multi-object spectroscopy, directly supporting studies of exoplanets, galaxy evolution, and dark energy. A key figure in bridging engineering and astronomy, Hare’s work ensures that observatories like GMT and Magellan remain at the forefront of discovery, making him an invaluable asset to the astronomical community.