Dr. Simon Radford
Wednesday, February 17, 2021
10:00am Arizona Time
The Submillimeter Array
The Submillimeter Array is the world's first imaging interferometric telescope for submillimeter astronomy, which reveals features of the universe invisible to the human eye. The SMA, located near the summit of Maunakea, one of the best observing sites in the world, comprises eight antennas that function together as one telescope. The SMA observes a wide variety of celestial objects, including: comets and planets in the Solar system; interstellar dust grains and molecular gas, often in cold, dense clouds where stars form; debris disks where planets form around young stars; the rich chemistry of interstellar material, especially around old, evolved stars; the distribution and structure of interstellar material in the Milky Way and in other galaxies; time variable compact objects, including active galactic nuclei; and the evolution of star formation in distant galaxies throughout the history of the universe.
About Dr. Radford
Simon Radford is Director of Hawaii Operations for the Submillimeter Array on Maunakea. Prior to joining the Smithsonian Astrophysical Observatory, he was a Member of the Professional Staff at the California Institute of Technology, where he was Technical Manager of the Caltech Submillimeter Observatory. Previously, he was a staff astronomer at the National Radio Astronomy Observatory in Tucson, Arizona, and at the Insitut de Radioastronomie Millimetrique in Grenoble, France. He received his B. S. in Engineering Physics from Cornell University and his M. S. and Ph. D. in Astronomy at the University of Washington. His research has included observations of the cosmic background radiation, spectroscopy of molecular gas in distant starburst galaxies, characterization of atmospheric conditions at submillimeter observing sites, and development of telescopes and instrumentation.