S. Ansoldi
University of Udine
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Featured researches published by S. Ansoldi.
Astronomy and Astrophysics | 2018
M. L. Ahnen; S. Ansoldi; L. A. Antonelli; C. Arcaro; D. Baack; A. Babic; B. Banerjee; P. Bangale; U. Barres de Almeida; J. A. Barrio; al.
The BL Lac object S5~0716+714, a highly variable blazar, underwent an impressive outburst in January 2015 (Phase A), followed by minor activity in February (Phase B). The MAGIC observations were triggered by the optical flux observed in Phase A, corresponding to the brightest ever reported state of the source in the R-band. The comprehensive dataset collected is investigated in order to shed light on the mechanism of the broadband emission. Multi-wavelength light curves have been studied together with the broadband Spectral Energy Distributions (SEDs). The data set collected spans from radio, optical photometry and polarimetry, X-ray, high-energy (HE, 0.1 GeV 100 GeV) with MAGIC. The flaring state of Phase A was detected in all the energy bands, providing for the first time a multi-wavelength sample of simultaneous data from the radio band to the VHE. In the constructed SED the textit{Swift}-XRT+textit{NuSTAR} data constrain the transition between the synchrotron and inverse Compton components very accurately, while the second peak is constrained from 0.1~GeV to 600~GeV by textit{Fermi}+MAGIC data. The broadband SED cannot be described with a one-zone synchrotron self-Compton model as it severely underestimates the optical flux in order to reproduce the X-ray to
arXiv: High Energy Astrophysical Phenomena | 2018
M. L. Ahnen; S. Ansoldi; L. A. Antonelli; C. Arcaro; A. Babic; B. Banerjee; P. Bangale; U. Barres de Almeida; J. A. Barrio; J. Becerra González; W. Bednarek; E. Bernardini; A. Berti; W. Bhattacharyya; O. Blanch; G. Bonnoli; R. Carosi; A. Carosi; Avishek Chatterjee; S. M. Colak; P. Colin; E. Colombo; Julio Contreras; J. Cortina; S. Covino; P. Cumani; P. Da Vela; F. Dazzi; A. De Angelis; B. De Lotto
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