Colloquia Schedule Fall 2013
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker This presentation being held at 3:00 pm during the Cosmos Seminar time-slot. |
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"The Present and Future of Exoplanets with Precise Radial Velocities" Pennsylvania State University host: Adam Kraus |
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Frank N. Bash Symposium 2013: New Horizons in Astronomy: 6-8 October 2013. No Colloquium presentation scheduled on 8 October, to avoid conflict. |
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Tinsley Visiting Scholar/Planetary Group "Accessing the Atmospheres of Terrestrial Exoplanets" Wesleyan University host: Michael Endl |
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"Large-Scale Surveys of Star Formation in the Milky Way" University of Florida host: Neal Evans |
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"Supermassive Black Hole Binaries: The Search Continues" Georgia Institute of Technology host: Steve Finkelstein |
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"Observational Hallmarks of Evolution and Planet Formation in Circumstellar Disks" Harvard-Smithsonian Center for Astrophysics host: Neal Evans |
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"The Role of Large Herschel Surveys in the Fields of Galaxy Evolution and Cosmology" California Institute of Technology host: Karl Gebhardt |
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"Galaxy Evolution at High Redshifts: Lyman-alpha and Other Lines" In the last few years we have progressed from merely finding Lyman-alpha galaxies to characterizing their physical properties using multiwavelength observations. After measuring their physical sizes, stellar and halo masses, ages, metallicities, dust properties and AGN fractions, we can now start to address why some (star-forming) galaxies at high redshift show bright Lyman-alpha emission whereas others don't? What is the escape fraction of Lyman-alpha photons? What helps these photons escape? Are these truly the youngest stages of galaxy formation? I will also discuss low-z line emitters that seem to lie outside the mass-metallicity and mass-star-formation relations. Arizona State University host: Steve Finkelstein |
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"Revealing Cosmic Origins: from Exoplanet Atmospheres to the Intergalactic Medium with the HST Cosmic Origins Spectrograph" University of Texas at Austin host: Edward Robinson |
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"A CMB Perspective of the Epoch of Reionization" University of California, Berkeley host: Paul Shapiro |
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"Dark Matter in the Smallest Galaxies" Carnegie-Mellon University host: Andrew Mann |
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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