13–15 May 2013
Union South
US/Central timezone

Session

High-Energy Gamma-Ray Astrophysics I

14 May 2013, 14:00
Union South

Union South

1308 West Dayton Street, Madison, WI 53706

Presentation materials

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  1. Mr Jonathan Dumm (UW-Madison)
    14/05/2013, 14:00
    High-Energy Gamma Ray Astrophysics Parallel
    The VERITAS observatory has now been operating for 5 years very successfully with >40 source detections in the TeV regime. A recent upgrade with high quantum efficiency photo detectors and a new camera trigger system sets the stage for the next phase of VERITAS. Key goals are to probe fundamental physics, including searches for dark matter annihilation signatures, to perform deep...
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  2. Dr Nicola Omodei (Stanford University/KIPAC)
    14/05/2013, 14:25
    High-Energy Gamma Ray Astrophysics Parallel
    After more than four years of science operation, the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope has detected more than 35 Gamma-Ray Bursts above 100 MeV. Fermi-LAT has provided a unique new dataset of high energy observations of Gamma-ray Bursts, which has led to many recent theoretical advancements and challenges. I will present an overview of the first 4 years of...
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  3. Elizabeth Hays (NASA GSFC)
    14/05/2013, 14:50
    High-Energy Gamma Ray Astrophysics Parallel
    In the past four years the Fermi Large Area Telescope (LAT) has detected a variety of Galactic sources of high energy gamma rays. Many of these source types were established or anticipated as gamma-ray emitters before the launch of Fermi, such as pulsars and their wind nebulae, supernova remnants, and high mass X-ray binaries. In these sources the LAT is revealing spectral details and for some...
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