Astronomy

Overview

Astronomy at University of British Columbia covers most areas of current interest in this broad field, including a wide range of theoretical and observational studies in astronomy, and also experimental and theoretical studies in cosmology. 

Research at optical wavelengths includes searches and orbital determination for asteroids and comets, photometric studies of stellar populations, particularly globular clusters, studies of distant galaxies and active galactic nuclei, and time-resolved spectroscopy of variable stars and active binary star systems. 

Key facts:

Studies at microwave and radio frequencies include research on variable radio sources, searches for pulsars, the early stages of star formation, relativistic jets, and balloon-borne measurements of the cosmic microwave background radiation. 

A variety of theoretical work complements this research, with topics that range from planetary dynamics and the structure of neutron stars, to theoretical studies of structure formation in the early universe. Development of astronomical instrumentation is also supported.

The Ph.D. in Physics or Astronomy program requires a thesis and 12 credits of coursework, all at the 500 level. The course selection is determined in consultation with the student's supervisory committee. Students entering the Ph.D. program must have the equivalent of the required courses for the M.Sc. program, or will be required to take those courses during the program.