Past Colloquia
Karl W. Kamper Memorial Lecture – Nearby Galaxy Mergers Seen with Adaptive Optics: A Sharper Image
Cody Hall
Claire E. Max (CfAO, UC Observatories)
December 06, 2013
14:00 - 15:00
Adaptive Optics is a technology that detects and corrects changing distortions in optical systems. It has been applied to great effect during the past decade for correcting astronomical telescopes for blurring due to turbulence in the Earth’s atmosphere. This talk will describe how Adaptive Optics works,…
CMB Polarization with the South Pole Telescope
Cody Hall
Duncan Hanson (McGill)
November 29, 2013
14:00 - 15:00
Measurements of polarization in the Cosmic Microwave Background (CMB) are our best hope to measure the amplitude and scale of gravity waves in the early Universe. They also have the power to provide an (astrophysical) determination of the absolute neutrino mass scale. For the past…
A Thermometer for Goldilocks: Accurate Temperatures of Kepler M Dwarfs and Their Planets
Cody Hall
Eric Gaidos (Hawaii)
November 22, 2013
14:00 - 15:00
M dwarf stars are especially attractive targets in the search for Earth-like planets because small planets are easier to detect around such stars, and the “habitable zone” is closer to the star where planets are more readily detected. The Kepler mission has discovered Earth-size planets…
Extragalactic Archeology
Cody Hall
Charlie Conroy (UC-Santa Cruz)
November 15, 2013
14:00 - 15:00
One of the main avenues for understanding the formation and evolution of galaxies is through studying their present day stellar populations. A new generation of population synthesis tools that we have been developing are now capable of extracting an unprecedented amount of information from high…
Higher Education Today: Outstanding Training for the Last Century
Cody Hall
David Helfand (Quest U)
November 08, 2013
14:00 - 15:00
Canada has the highest post-secondary participation rate among OECD countries, and yet one of the lowest innovation rates. Why? I will offer an irreverent critique of “modern” universities and provide a description of a provocative alternative in Canada’s first independent, not-for-profit secular institution, Quest University…
Searching for Ghosts at SNOLAB
Cody Hall
Mark Chen (Queens)
November 01, 2013
14:00 - 15:00
SNOLAB is Canada’s world-leading underground laboratory for particle astrophysics experiments. What are we trying to do there? Detect the invisible: searching for particles of dark matter, measuring the flux of ghostly neutrinos from the Sun and the Earth, trying to observe a most peculiar nuclear…
Massive Stars Across the Cosmos: Engines, Lighthouses, and Laboratories
Cody Hall
Emily Levesque (Colorado)
October 25, 2013
14:00 - 15:00
Massive stars can provide valuable information on a Galactic, extragalactic, and even cosmological scale. The radiative signatures observed in HII regions and star-forming galaxies are determined by massive stellar populations. Long-duration gamma-ray bursts, produced during the core-collapse deaths of unusual massive stars, can be utilized as powerful probes of the…
Galaxy mergers in the nearby universe
Cody Hall
Sara Ellison (University of Victoria)
October 21, 2013
14:00 - 15:00
Galaxy mergers are known to trigger dramatic changes in galactic morphology, metallicity, star formation and black hole accretion rates. However, the extent to which these properties respond to the interaction can vary greatly both between different mergers, and at different times during a given interaction. …
Astrophysics with Submillimeter Galactic Plane Surveys
Cody Hall
Yancy Shirley (Arizona)
October 11, 2013
14:00 - 15:00
The advent of large format bolometers arrays have made it possible to survey the Galaxy and search for embedded sites of star formation in a much less biased way than previous studies. The Bolocam Galactic Survey (BGPS) is a continuum survey 1.1 mm at 30″…
The formation of supermassive black holes in the universe
Cody Hall
Priya Natarajan (Yale)
October 04, 2013
14:00 - 15:00
Populations of quasars powered by accretion onto SMBHs with masses in excess of 10^9 solar masses are now detected when the Universe was barely a Gyr old. And in the local universe the centers of several nearby brightest cluster galaxies harbor behemoths that weigh ~ a…