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Gamma-ray Burst Studies Using the H.E.S.S. Cherenkov Array


Speaker:Dr. P.H. Tam
Affiliation:Landessternwarte, Universität Heidelberg, Königstuhl
Date:January 21, 2009 (Wed)
Time:4:00-5:00 p.m.
Venue:Room 522, 5/F, Chong Yuet Ming Physics Building, HKU

Abstract:

Without prior signal, an enormous amount of energy is released for seconds in Gamma-ray bursts (GRBs). The emitting regions can produce Very-High-Energy (VHE) gamma-ray photons of energy ~1011 eV during and after the burst. These VHE gamma-rays may be attenuated in the source or by the extragalactic background light (EBL). After a brief review on the current status of VHE observations of GRBs, the ground-based H.E.S.S. array of four imaging atmospheric Cherenkov telescopes (IACT), sensitive to VHE gamma-rays, is introduced. H.E.S.S. observations of 34 GRBs were carried out during 2003-2008. No evidence of VHE gamma-rays was found. Flux upper limits derived for GRB 030329 and GRB 060505 are compared and are found consistent with the synchrotron self-Compton flux calculated in the context of relativistic blast-wave model. The case of GRB 060602B where strictly simultaneous observations with H.E.S.S. throughout the GRB duration is highlighted. Some future prospects of VHE gamma-ray observations of GRBs are discussed.

Coffee and tea will be served 20 minutes prior to the seminar.