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Paper: |
Synchrotron-Self Compton Spectral Evolution of PKS 2155-304 |
Volume: |
299, High Energy Blazar Astronomy |
Page: |
269 |
Authors: |
Ciprini, S.; Tosti, G. |
Abstract: |
The high frequency peaked blazar PKS 2155-304 is one of the brightest and most intensively studied prototype of BL Lac objects. Gamma-rays from PKS 2155-304 have been detected from the MeV to TeV ranges. We computed a synchrotron self-Compton (SSC) model, based on the temporal behavior of the particles distribution, responsible for the high-energy emission. Using the available simultaneous multiwavelength data, we simulated the overall spectral energy distribution (SED) and the spectral variability of this source. |
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