2016 - 2017 Astro Seminar Schedule

DateEvent TypeSpeakerTitle
09/23/2016Astro SeminarAshley ZaudererObservational Signatures of Tidal Disruption Events: Are Jets and Radio Emission Ubiquitous? [ + Description ]
09/30/2016Astro SeminarZoltan HaimanRapid Formation of the First Supermassive Black Holes [ + Description ]
10/07/2016Astro SeminarPeter GarnavichThe Earliest Hours of Supernovae with Kepler/K2 [ + Description ]
10/21/2016Astro SeminarRachel SommervilleThe impact of AGN driven winds on galaxy quenching, morphology, and structure [ + Description ]
11/04/2016Astro SeminarAdrian LiuThe Past, Present, and Future of 21cm Cosmology [ + Description ]
11/11/2016Astro SeminarPieter van DokkumExploring the low surface brightness sky with the Dragonfly Telephoto Array [ + Description ]
11/18/2016Astro SeminarJo BovyStellar streams and fundamental physics [ + Description ]
12/02/2016Astro SeminarSjoert van VelzenNew ways to study the tidal disruption of stars by supermassive black holes [ + Description ]
01/23/2017Astro SeminarMaryam ModjazStellar Forensics with the Most Powerful Explosions in the Universe [ + Description ]
01/27/2017Big Apple ColloquiumHiranya PeirisTowards Fundamental Physics from the Cosmic Microwave Background [ + Description ]
02/03/2017Astro SeminarPhilipp MoestaModeling the most powerful explosions in 3D [ + Description ]
02/10/2017Astro SeminarBenoit CotéConnecting Nuclear Astrophysics to Cosmological Structure Formation with Galactic Chemical Evolution [ -- Description ]

Description: Detailed stellar abundances from modern astronomical surveys represent a novel window on the early universe and on the formation of the Milky Way and its satellite galaxies. However, the theoretical tools needed to translate these abundances into meaningful understanding of cosmological structure formation are challenged by uncertainties in their inputs. To address this fundamental challenge, we created a flexible pipeline for modeling chemical evolution which connects nuclear physics, stellar evolution, galaxy evolution, astronomical observations, and cosmology. In this talk, I will present how our codes, along with statistical tools, can be used to quantify the reliability of numerical predictions and to constrain the origin of light and heavy elements in the universe. The multidisciplinary nature of this research allows to develop new intersections between nuclear astrophysics, gravitational wave physics, and cosmology. Our ultimate goal is to confidently use stellar abundances as tracers to better understand how galaxies form and evolve. (11:00 AM, 726 Broadway, 940, CCPP Seminar)
02/17/2017Astro SeminarOr GraurRage against the dying of the light: what can we learn from three-year-old supernovae? [ + Description ]
03/10/2017Astro SeminarAna BonacaThe Milky Way halo in the Gaia era [ + Description ]
03/17/2017Astro Seminarn/ano astro seminar -- Spring Break [ + Description ]
03/24/2017Astro Seminarn/ano astro seminar -- prospective graduate student day [ + Description ]
03/31/2017Astro SeminarEmanuele CastorinaCosmology with Neutral Hydrogen [ + Description ]
04/07/2017Astro SeminarColin HillNew Information in Ancient Photons: Novel Approaches to CMB Secondary Anisotropies [ + Description ]
04/21/2017Astro SeminarEliot Quataert [ + Description ]
04/28/2017Astro SeminarAndy Howel [ + Description ]
05/05/2017Astro SeminarTjitske StarkenburgTBA [ + Description ]