Colloquia Schedule Fall 2014
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
"Hot Chromospheres and Flares on Cool and Ultracool Dwarfs" Ohio State University host: Adam Kraus |
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"Let it Collide: An Epic Saga of Star Wars Planets, Planetesimals, and Super Planet Crashes" University of Texas at Austin host: Adam Kraus |
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"The Complex Interplay between Star Formation and Galaxy Evolution from z~0-6" Haverford College host: Steve Finkelstein |
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"Compact Galaxies and Super-Massive Black Holes" Max Planck Institute for Astronomy (MPIA), Heidelberg host: Karl Gebhardt |
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"The Architecture and Timing of Planetary Systems" University of Chicago host: TBD |
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"Who's Afraid of the Big Bad Supermassive Black Hole?" Pennsylvania State University host: Steve Finkelstein |
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"Puzzles in the Structure of Disk Galaxies" Queen's University, Kingston, Ontario, Canada host: Karl Gebhardt |
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"Galaxy Build-up in the First Gyr: Insights from ultra-deep HST and Spitzer Observations" Yale University host: Steve Finkelstein |
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"Forming Earths and Mercuries: Solids Less Volatile than Ice" American Museum of Natural History, New York host: Joel Green |
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"Shedding Lyman Alpha Light on Cosmological Reionization" Arizona State University host: Steve Finkelstein |
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"From Disks to Planets: Observational Insights" Rice University host: Adam Kraus |
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"The Giant Magellan Telescope Project: Science and Status" Giant Magellan Telescope (GMT) host: Taft Armandroff |
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"There's Government in Your Science" American Astronomical Society host: Jeff Silverman |
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DeVaucouleurs Medalist DeVaucouleurs Lecture: "The Growth of Supermassive Black Holes and Galaxy Evolution" Multiwavelength surveys like GOODS and COSMOS indicate that most actively growing black holes are heavily obscured, and this fraction increases in the young Universe and in lower luminosity AGN. Most black holes grow in moderate luminosity AGN, which dominate the X-ray "background," rather than in luminous quasars. In the peak epoch of black hole growth, at z~1-3, such AGN are hosted in galaxies with significant disks, and thus cannot have undergone a recent major merger. Using morphological classifications from Galaxy Zoo (at z~0), we identify two distinct modes of galaxy evolution, with mergers and AGN feedback affecting only a minority. Mergers are more important at the high luminosity end, i.e., in quasars. Using a large-area hard X-ray survey ("Stripe 82X"), which finds quasars even in obscured systems, we are starting to fill in the last missing piece of a complete census of black hole growth across the luminous Universe. Yale University dinner host: Shardha Jogee (Medal Awarded by Daniel Jaffe) |
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DeVaucouleurs Medalist Public Lecture: "Black Holes, Galaxies and the Evolution of the Universe: An Observer's View" Yale University dinner host: Daniel Jaffe |
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DeVaucouleurs Medalist UT CNS Women in Science Lecture: "Why So Few? The Dearth of Women in Science" Yale University dinner host: Dean Linda Hicke |
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"Brown Dwarfs as Exoplanet Analogs" Bucknell University, Lewisburg PA host: Adam Kraus |
Visitors to the Department of Astronomy can find detailed information and maps on our Visiting Austin Page.
Please report omissions/corrections to: G. Orris at argus@astro.as.utexas.edu.
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