MAGIC upper limits on the GRB 090102 afterglow

J Aleksic,S Ansoldi,L Antonelli,P Antoranz,A Babic,P Bangale,U Barres De Almeida,J A Barrio,J Becerra Gonzalez,W Bednarek,K Berger,E Bernardini,A Biland,O Blanch,R Bock,S Bonnefoy,G Bonnoli,F Borracci,T Bretz,E Carmona,A Carosi,D Carreto Fidalgo,P Colin,E Colombo,J L Contreras,J Cortina,S Covino,P Da Vela,F Dazzi,A De Angelis,G De Caneva,B De Lotto,C Delgado Mendez,M Doert,A Dominguez,D Dominis Prester,D Dorner,M Doro,S Einecke,D Eisenacher,D Elsaesser,E Farina,D Ferenc,M V Fonseca,L Font,K Frantzen,C Fruck,R J Garcia Lopez,M Garczarczyk,D Garrido Terrats,M Gaug,G Giavitto,N Godinovic,A Gonzalez Munoz,S R Gozzini,D Hadasch,M Hayashida,A Herrero,D Hildebrand,J Hose,D Hrupec,W Idec,V Kadenius,H Kellermann,M L Knoetig,K Kodani,Y Konno,J Krause,Hiroshi Kubo,J Kushida,A La Barbera,D Lelas,N Lewandowska,E Lindfors,S Lombardi,M Lopez,R Lopezcoto,A Lopezoramas,E Lorenz,Irene Albarran Lozano,M Makariev,K Mallot,G Maneva,N Mankuzhiyil,K Mannheim,L Maraschi,B Marcote,M Mariotti,M Martinez,D Mazin,U Menzel,M Meucci,J M Miranda,R Mirzoyan,A Moralejo,P Munaradrover,D Nakajima,A Niedzwiecki,K Nilsson

Monthly Notices of the Royal Astronomical Society（2014）

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摘要

Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Energetic Gamma-Ray Experiment Telescope observations during the 1990s and they have been confirmed by the data of the Fermi satellite. These results have, however, shown that our understanding of GRB physics is still unsatisfactory. The new generation of Cherenkov observatories and in particular the MA...

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关键词

radiation mechanisms: non-thermal,gamma-ray burst: general

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