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Mario Mateo observes the stars and motion of objects in nearby galaxies to assess the distribution of mass, particularly dark mass, within them. He is a ground-breaking instrumentalist, who has designed and built fiber spectrographs for Magellan that can analyze an unprecedented number of targets – more than 250 – at a time. His new Michigan/Magellan Fiber System (M2FS) is the most powerful yet and is ideal for studying objects’ chemical composition, mass, temperature, and motion. It has uniquely positioned Mateo’s group to follow up on the deluge of new detections expected from sky surveys like the LSST, Dark Energy Survey, and SkyMapper. Student Jeb Bailey plans to use it to study hot Jupiters, and Mateo plans to explore the evolution of dwarf galaxies and their interactions with the Milky Way.
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Astronomical Society of the Pacific Conference Series (2018): 99-103
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