Direct Detection of Extra-solar Planets Using High Contrast Imaging
James R. Graham
University of Toronto

Large astronomical telescopes coupled with new adaptive optics technologies enable high contrast imaging. Current systems approach a dynamic range of nearly a million to one on scales near the diffraction limit. In the next decade a new generation of instruments will improve contrast by another one to two orders of magnitude and provide images of extra-solar planetary systems.

Date:	Mardi, 8 mars 2011
Time:	16:00
Where:	McGill University
	Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
Contact:	Robert Rutledge