MAGIC observations of the February 2014 flare of 1ES 1011+496 and ensuing constraint of the EBL density

M. L. Ahnen; S. Ansoldi; L. A. Antonelli; P. Antoranz; A. Babic; B. Banerjee; P. Bangale; U. Barres de Almeida; J. A. Barrio; J. Becerra González; W. Bednarek; E. Bernardini; B. Biasuzzi; A. Biland; O. Blanch; S. Bonnefoy; G. Bonnoli; F. Borracci; T. Bretz; E. Carmona; A. Carosi; A. Chatterjee; R. Clavero; P. Colin; E. Colombo; J. L. Contreras; J. Cortina; S. Covino; P. Da Vela; F. Dazzi; A. De Angelis; B. De Lotto; E. de Oña Wilhelmi; C. Delgado Mendez; F. Di Pierro; D. Dominis Prester; D. Dorner; M. Doro; S. Einecke; D. Eisenacher Glawion; D. Elsaesser; A. Fernández-Barral; D. Fidalgo; M. V. Fonseca; L. Font; K. Frantzen; C. Fruck; D. Galindo; R. J. García López; M. Garczarczyk; D. Garrido Terrats; M. Gaug; P. Giammaria; N. Godinović; A. González Muñoz; D. Guberman; A. Hahn; Y. Hanabata; M. Hayashida; J. Herrera; J. Hose; D. Hrupec; G. Hughes; W. Idec; K. Kodani; Y. Konno; H. Kubo; J. Kushida; A. La Barbera; D. Lelas; E. Lindfors; S. Lombardi; F. Longo; M. López; R. López-Coto; A. López-Oramas; E. Lorenz; P. Majumdar; M. Makariev; K. Mallot; G. Maneva; M. Manganaro; K. Mannheim; L. Maraschi; B. Marcote; M. Mariotti; M. Martínez; D. Mazin; U. Menzel; J. M. Miranda; R. Mirzoyan; A. Moralejo; E. Moretti; D. Nakajima; V. Neustroev; A. Niedzwiecki; M. Nievas Rosillo; K. Nilsson; K. Nishijima; K. Noda; R. Orito; A. Overkemping; S. Paiano; J. Palacio; M. Palatiello; D. Paneque; R. Paoletti; J. M. Paredes; X. Paredes-Fortuny; M. Persic; J. Poutanen; P. G. Prada Moroni; E. Prandini; I. Puljak; W. Rhode; M. Ribó; J. Rico; J. Rodriguez Garcia; T. Saito; K. Satalecka; C. Schultz; T. Schweizer; S. N. Shore; A. Sillanpää; J. Sitarek; I. Snidaric; D. Sobczynska; A. Stamerra; T. Steinbring; M. Strzys; L. Takalo; H. Takami; F. Tavecchio; P. Temnikov; T. Terzić; D. Tescaro; M. Teshima; J. Thaele; D. F. Torres; T. Toyama; A. Treves; V. Verguilov; I. Vovk; J. E. Ward; M. Will; M. H. Wu; R. Zanin

doi:10.1051/0004-6361/201527256

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Volume 590 (June 2016)

A&A, 590 (2016) A24

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Fig. 3

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Evolution of the photon index from power-law fits to the de-absorbed night-wise spectra of 1ES 1011+496 between February 6 and March 7 2014. The error bars are the parameter uncertainties from the fits. The red line represents the fit to a constant value, for which the probability is 10%.

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