Very-high-energy γ-rays from the universe middle age: Detection of B0218+357 and PKS1441+25 with the MAGIC telescopes

Bibcode
2017AIPC.1792e0035N
DOI
10.1063/1.4968981
Nievas Rosillo, M.; Becerra González, J.; Buson, Sara; González, José Luis Contreras; Presler, Dijana Dominis; Manganaro, M.; Sitarek, Julian; Tavecchio, Fabrizio; MAGIC Collaboration; Fermi-LAT Collaboration
Referencia bibliográfica

AIP Conference Proceedings, Volume 1792, Issue 1, id.050035

Fecha de publicación:
1
2017
Revista
AIP Conference Proceedings
Número de autores
10
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
Out of the ˜ 70 extragalactic sources known to emit in the Very High Energy band (VHE, E > 100GeV), only 5-6 are known to be Flat Spectrum Radio Quasars (FSRQs), and they are all found at intermediate or high redshifts. In this paper, we explore the conditions that trigger sub-TeV emission on this particular type of sources and we concentrate on the two most distant examples of this special population of blazars: the gravitationally lensed quasar B0218+357 and PKS 1441+25.
Tipo
Sin árbitro

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