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    Simultaneous observations of the blazar PKS 2155-304 from ultra-violet to TeV energies

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    Simultaneous_observations_of_the blazar_PKS_ 2155−304.pdf (899.7Kb)
    Date
    2020
    Author
    Abdalla, H.
    Arcaro, C.
    Backes, M.
    Barnard, M.
    Böttcher, M.
    Chand, T.
    Chandra, S.
    Kreter, M.
    Ndiyavala, H.
    Schutte, H.M.
    Seyffert, A.S.
    Van der Walt, D.J.
    Van Rensburg, C.
    Venter, C.
    Wadiasingh, Z.
    Zacharias, M.
    Zywucka, N.
    H.E.S.S. Collaboration
    Fermi LAT
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    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
    URI
    http://hdl.handle.net/10394/35526
    https://www.aanda.org/articles/aa/pdf/2020/07/aa36900-19.pdf
    https://doi.org/10.1051/0004-6361/201936900
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