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catch a burst and notify other observatoriesboth in space and on the ground of its approximate locationWithin minutes HETE2 mayobtain a precise locationCurrent telescopestake much longer to notify o. Alexander . Kotov. , . ChengXiang. . Zhai. , Richard . Sproat. University of Illinois at Urbana-Champaign. Roadmap. Problem definition. Previous work. Approach. Experiments. Summary. Motivation. Web data is generated by a large number of textual streams (news, blogs, tweets, etc. . . . . . Maria . Giovanna Dainotti. Stanford . University, USA, Fulbright Scholar, . now . JSPS Fellow . at . Riken, Tokyo, . extreme physics at play. Bruce Gendre. ARTEMIS. Description of a GRB. Gamma-ray Burst : . burst of high energy photons. Isotropic distribution on the sky. extragalactic events. . quite common (~2/day. Gamma ray bursts (GRB) are an especially exciting outflow phenomena that are capable of outputting as much energy as our sun will. Christopher C. . Lindner. 1. Abstract. Relativistic Jets are streams of plasma moving throughout the universe at speeds up to 99% the speed of light. They produce high-energy X-ray, radio, and visible radiation that are observable from great distances across the universe. Andrew Levan. University of Warwick. Parameter space. Kouveliotou. et al. 1993. Parameter space. Kulkarni. & . Kasliwal. 2010. Parameter space. LGRBs. SGRBs. SGRs. ?. TDEs?. Galactic sources (SGR, LMXB, HMXB, . Manel. Martinez. 4. 3. rd. . Winter Meeting. March 2015-Benasque. Outline. 1) Introduction. 2) Basics on VHE Gamma Astronomy physics. 3) VHE gamma observatories. 4) CTA. 5. ) Conclusions. 1) INTRODUCTION. Radiation-Dominated Jet?. Kunihito. . Ioka. (KEK). T. Inoue, Asano & KI, . arXiv. : 1011.6350. KI. , . arXiv. : 1006.3073. Suwa. & KI, . arXiv. : 1009.6001. KI+, in . preparation (. Andrew Levan. University of Warwick. Burst durations. Swift 1644+57. Very long bursts are often image triggers (1000+s). Correction from Swift observed rates to astrophysical rates (at Swift limits) could be a factor 10. Yun. -Wei YU. 俞云伟. June 22, 2010, Hong Kong. Outline. Background. Implications from the shallow decay afterglows of GRBs. A qualitative discussion on . magnetar. wind emission. Emission from the termination shock of the wind. Edwin Kite (U. Chicago), John Armstrong (Weber State), . Robin Wordsworth (Harvard), Francois Forget (LMD) . c. an climate . models. h. elp distinguish. these scenarios?. h. abitable surface. s. terile surface. Mysterious explosions in the Universe. Poonam Chandra. Royal Military College of Canada. Universe is 14 billion years old.. Our sun is 5 billion years.. Supernovae and Gamma ray bursts. Explosions lasting fraction of a second to few seconds.. from keV to . GeV. energies and . beyond. . Elisabetta Bissaldi. Member of the Fermi-GBM and . Fermi-LAT Collaborations, . and of the CTA Consortium. Politecnico. . & INFN . Bari. elisabetta.bissaldi@ba.infn.it. Liz Hays . (. NASA Goddard Space Flight Center). The Origin of Cosmic Rays. Credit S. . Swordy. Victor Hess and his . “Flight . Ops . Team”, . 1912. From protons. Pion decay. Accelerated protons (p) interact with matter. National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) .