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The Astronomy M.S. and Ph.D. programs aim to equip students for careers in astronomical or astrophysical research or university-level teaching. Each student follows a personalized curriculum designed by their advisor and advisory committee. For the M.S. degree, we provide two pathways: a coursework-based option where students complete graduate-level astronomy classes and pass an examination, and a thesis option that teaches students to develop, execute, and document research projects. Ph.D. candidates must produce original, independent research.
Learning Outcomes
Master graduate-level astrophysics concepts.
Achieve graduate-level proficiency in either classical mechanics, quantum theory, or electromagnetic theory.
Develop expertise in mathematical physics at the graduate level.
Gain proficiency in observational astronomy methods.
Understand the astrophysics of gaseous nebulae, active galactic nuclei, and high-energy astrophysics.
Acquire graduate-level knowledge of cosmology.