Detecting extended gamma-ray emission with the next generation Cherenkov telescopes

Very high energy (VHE >100 GeV) gamma rays coming from blazars can produce pairs when interacting with the Extragalactic Background Light (EBL) and the Cosmic Microwave Background, generating an electromagnetic cascade. Depending on the Intergalactic Magnetic Field (IGMF) intensity, this cascade...

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Detalles Bibliográficos
Publicado:	2015
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso http://hdl.handle.net/20.500.12110/paper_18248039_v30-July-2015_n_p_Alonso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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