Name: Science with the New Generation of High Energy Gamma-Ray Experiments #6
Start: 2008-10-08T08:00:00+02:00
End: 2008-10-10T20:00:00+02:00
Location: Padova

Science with the New Generation of High Energy Gamma-Ray Experiments #6

from Wednesday, October 8, 2008 (8:00 AM) to Friday, October 10, 2008 (8:00 PM)

Monday, October 6, 2008
Tuesday, October 7, 2008
Wednesday, October 8, 2008
2:30 PM
2:30 PM - 4:30 PM
Room: Aula A - Physics Dept. - Padova University
Contributions

3:50 PM GeV - TeV Multiwavelength Opportunities - David Thompson (NASA Goddard Space Flight Center, on behalf of the Fermi LAT collaboration)
Thursday, October 9, 2008
9:00 AM
9:00 AM - 11:00 AM
Room: Centro Congressi Pietro d'Abano
Contributions

10:00 AM Status and recent results of MAGIC - Javier Rico (ICREA/IFAE)

10:30 AM VERITAS - Status and results of the 2007/2008 season - Matthias Beilicke (Washington University)
11:00 AM coffee break
coffee break
11:00 AM - 11:20 AM
11:30 AM
11:30 AM - 12:50 PM
Contributions

11:30 AM The time evolution of pulsar wind nebulae in the GeV-TeV domain - Ocker Cornelis de Jager (North-West University, Potchefstroom, South Africa)

11:50 AM Massive stars in colliding wind systems: the high-energy gamma-ray perspective - Anita Reimer (Stanford University)

12:10 PM Supernova remnants interact with molecular clouds and reveal accelerated hadrons - Fabrice Feinstein (Université Montpellier 2)

12:30 PM The GeV to TeV view of SNR IC443: predictions for GLAST - Ana Yaiza Rodriguez Marrero (IEEC-CSIC)
12:50 PM lunch
lunch
12:50 PM - 2:30 PM
2:30 PM
2:30 PM - 3:40 PM
Contributions

2:45 PM Detection of pulsed gamma rays above 25 GeV from the Crab Pulsar with the MAGIC Telescope - Maxim Shayduk (Max-Planck-Institut fuer Physik, D-80805 Muenchen) Michael Rissi (ETH Zuerich, CH-8093 Switzerland)

3:05 PM Fermi Gamma-ray Space Telescope Observations of Gamma-ray Pulsars - Pablo Saz Parkinson (University of California, Santa Cruz)
3:40 PM
3:40 PM - 4:20 PM
Contributions

4:00 PM Formation of hard VHE gamma-ray spectra of blazars due to internal photon-photon absorption - Dmitry Khangulyan (MPI f. Kernphysik, Heidelberg)
4:20 PM coffee break
coffee break
4:20 PM - 4:50 PM
4:50 PM
4:50 PM - 6:30 PM
Contributions

4:50 PM The blazar sequence: prospects for GeV and TeV observations - Fabrizio Tavecchio (INAF)

5:20 PM Gamma ray emission and particle acceleration in galaxy clusters - Gianfranco Brunetti (INAF-IRA, Bologna)

6:10 PM Constraints on Extragalactic Background Light from Cherenkov telescopes: status and perspectives for the next 5 years - Daniel Mazin (IFAE, Barcelona)
8:30 PM social dinner at "La Piroga", Selvazzano Dentro - Padova
social dinner at "La Piroga", Selvazzano Dentro - Padova
8:30 PM - 8:31 PM
Friday, October 10, 2008
9:00 AM
9:00 AM - 11:00 AM
Contributions

9:00 AM The hunt for cosmic sources with IceCube - Elisa Bernardini (DESY)
11:00 AM coffie break
coffie break
11:00 AM - 11:30 AM
11:30 AM
11:30 AM - 12:50 PM
Contributions

11:50 AM GRB observations with new generation IACTs in the GLAST era - Stefano Covino (INAF / Brera)

12:30 PM Exploring Quantum Gravity with Very-High-Energy Gamma-Ray Instruments - Prospects and Limitations - Robert Wagner (Max-Planck-Institut für Physik, München)
12:50 PM lunch
lunch
12:50 PM - 2:30 PM
2:30 PM
2:30 PM - 4:30 PM
Contributions

3:00 PM GRIPS: Gamma-Ray Burst Investigation via Polarimetry and Spectroscopy - Kanbach Gottfried (MPE, Garching)

3:50 PM Indirect search for Dark Matter with Fermi from the Galactic Center - Vincenzo Vitale (Dip. Fisica Roma 2)

4:10 PM Cosmic Ray Nuclei in the Galaxy and their secondary products: a new comprehensive model. - Dario Grasso (INFN, Pisa)
4:30 PM break
break
4:30 PM - 5:00 PM
5:00 PM
5:00 PM - 5:40 PM
Contributions

5:00 PM Acceleration of UHE Protons at Cluster Accretion Shocks and Related Non-thermal Emission - Giulia Vannoni (Max-Planck-Institut für Kernphysik, Heidelberg)

5:20 PM On the level of the cosmic ray sea flux. - Sabrina Casanova (Max Planck fuer Kernphysik)
5:40 PM concluding remarks
concluding remarks
5:40 PM - 5:55 PM

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