Insights into the emission of the blazar 1ES 1011+496 through unprecedented broadband observations during 2011 and 2012

J. Aleksić; S. Ansoldi; L. A. Antonelli; P. Antoranz; C. Arcaro; A. Babic; 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; 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; E. de Oña Wilhelmi; C. Delgado Mendez; F. Di Pierro; D. Dominis Prester; D. Dorner; M. Doro; S. Einecke; D. Eisenacher; 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; N. Godinović; A. González Muñoz; S. R. Gozzini; D. Hadasch; Y. Hanabata; M. Hayashida; J. Herrera; J. Hose; D. Hrupec; W. Idec; V. Kadenius; H. Kellermann; M. L. Knoetig; K. Kodani; Y. Konno; J. Krause; H. Kubo; J. Kushida; A. La Barbera; D. Lelas; N. Lewandowska; E. Lindfors; S. Lombardi; F. Longo; M. López; R. López-Coto; A. López-Oramas; E. Lorenz; I. Lozano; M. Makariev; K. Mallot; G. Maneva; K. Mannheim; L. Maraschi; B. Marcote; M. Mariotti; M. Martínez; D. Mazin; U. Menzel; J. M. Miranda; R. Mirzoyan; A. Moralejo; P. Munar-Adrover; D. Nakajima; V. Neustroev; A. Niedzwiecki; M. Nievas Rosillo; K. Nilsson; K. Nishijima; K. Noda; R. Orito; A. Overkemping; S. Paiano; M. Palatiello; D. Paneque; R. Paoletti; J. M. Paredes; X. Paredes-Fortuny; M. Persic; J. Poutanen; P. G. Prada Moroni; E. Prandini; I. Puljak; R. Reinthal; W. Rhode; M. Ribó; J. Rico; J. Rodriguez Garcia; T. Saito; K. Saito; K. Satalecka; V. Scalzotto; V. Scapin; 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; P. Vogler; M. Will; R. Zanin; S. Buson; F. D’Ammando; A. Lähteenmäki; T. Hovatta; Y. Y. Kovalev; M. L. Lister; W. Max-Moerbeck; C. Mundell; A. B. Pushkarev; E. Rastorgueva-Foi; A. C. S. Readhead; J. L. Richards; J. Tammi; D. A. Sanchez; M. Tornikoski; T. Savolainen; I. Steele

doi:10.1051/0004-6361/201527176

Home

All issues

Volume 591 (July 2016)

A&A, 591 (2016) A10

Full HTML

Free Access

Fig. 5

Open with DEXTER Download original image

Fractional variability amplitude, F_var as a function of frequency for data simultaneous to the MAGIC observation periods (left) shown in Fig. 3 and long-term data samples (right) shown in Fig. 4. The F_var of the radio core (right) is indicated by an open circle, while the values computed for the components C1 to C5 are represented by filled symbols (C1: circle; C2: upward triangle; C3: star; C4: downward triangle; C5: square).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.