Colloquia Schedule Fall 2016
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
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Setting Stellar Chronometers: The PTF(+) Open Cluster Survey Columbia University host: Adam Kraus |
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Exploring Galaxy Formation in the Epoch of Reionisation University of Sussex host: Steve Finkelstein |
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The Milky Way Laboratory Harvard-Smithsonian Center for Astrophysics host: Neal Evans |
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No talk scheduled |
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Spin and Magnetism in Cool Stars Massachusetts Institute of Technology Kavli Institute for Astrophysics and Space Research host: Andrew Mann |
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A Story of Stellar Nurseries Harvard-Smithsonian Center for Astrophysics host: Caitlin Casey |
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Network Cosmology: What can we learn from galaxy Facebook? Comet Update! The Fossil Record of Binary and Planetary Orbits UT Postdocs (Three talks) |
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Formation and Compositions of Planet Interiors and Atmospheres: Discoveries from Kepler, K2, and beyond California Institute of Technology host: Brendan Bowler |
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The Future of Exoplanet Science at McDonald Observatory Penn State University host: Greg Mace |
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Building Supermassive Black Hole Binaries Vanderbilt University host: Craig Wheeler/Eva Noyola |
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Towards the Characterization of Potentially Habitable Planets with High Resolution Spectroscopy University of Colorado Boulder host: Dan Jaffe |
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Controlling Star Formation: From Clouds to Galaxies Princeton University host: Volker Bromm |
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Drilling the Chicxulub Impact Structure: Study of large impact formation and effects on life The University of Texas at Austin Institute for Geophysics host: Bill Cochran |
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Dust-obscured star formation at the Cosmic Frontier : New observations from the Large Millimeter Telescope While UV surveys have mapped out the unobscured star formation rate density over cosmic time, our observations of obscured star formation remain incomplete beyond z~3. Millimeter observations are crucial to complete the census of star formation in the Universe. I will present new observations with the Large Millimeter Telescope including a 1.1 mm survey of the HST Frontier Fields. The clusters act as cosmic telescopes to amplify lower-luminosity galaxies, probing further down the millimeter luminosity function than possible with blank-field observations. With this survey we detect dust in galaxies with star formation rates as low as ~10 solar masses per year allowing us to measure the dust-obscured star formation in typical galaxies at high redshift. I will highlight an curious galaxy which challenges our picture of dust obscuration in the early Universe. University of Massachusetts Amherst host: Caitlin Casey |
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Moving Near Field Cosmology Beyond the Local Group Texas Tech University host: Kristy McQuinn |
Visitors to the Department of Astronomy can find detailed information and maps on our Visiting Austin Page.
Please report omissions/corrections to: visitor@astro.as.utexas.edu.
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