Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/127270
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Type: Journal article
Title: Simultaneous observations of the blazar PKS 2155-304 from ultra-violet to TeV energies
Author: Abdalla, H.
Adam, R.
Aharonian, F.
Benkhali, F.A.
Anguner, E.O.
Arakawa, M.
Arcaro, C.
Armand, C.
Ashkar, H.
Backes, M.
Martins, V.B.
Barnard, M.
Becherini, Y.
Berge, D.
Bernlohr, K.
Blackwell, R.
Bottcher, M.
Boisson, C.
Bolmont, J.
Bonnefoy, S.
et al.
Citation: Astronomy and Astrophysics: a European journal, 2020; 639:A42-1-A42-13
Publisher: EDP Sciences
Issue Date: 2020
ISSN: 0004-6361
1432-0746
Statement of
Responsibility: 
H. Abdalla … R. Blackwell …. P. deWilt … K. Feijen … G. Rowell … et al.
Abstract: Here we report the results of the first ever contemporaneous multi-wavelength observation campaign on the BL Lac object PKS 2155−304 involving Swift, NuSTAR, Fermi-LAT, and H.E.S.S. The use of these instruments allows us to cover a broad energy range, which is important for disentangling the different radiative mechanisms. The source, observed from June 2013 to October 2013, was found in a low flux state with respect to previous observations but exhibited highly significant flux variability in the X-rays. The high-energy end of the synchrotron spectrum can be traced up to 40 keV without significant contamination by high-energy emission. A one-zone synchrotron self-Compton model was used to reproduce the broadband flux of the source for all the observations presented here but failed for previous observations made in April 2013. A lepto-hadronic solution was then explored to explain these earlier observational results.
Rights: © H. Abdalla et al. 2020. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
DOI: 10.1051/0004-6361/201936900
Grant ID: ARC
Published version: http://dx.doi.org/10.1051/0004-6361/201936900
Appears in Collections:Aurora harvest 4
Physics publications

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