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Blazar Variability from Turbulence in Jets Launched by Magnetically Arrested Accretion Flows

  • Authors: Michael O' Riordan, Asaf Pe'er, and Jonathan C. McKinney

2017 The Astrophysical Journal 843 81.

  • Provider: AAS Journals

Caption: Figure 4.

γ-ray light curve (frequency integrated between 1019 and 1024 Hz) with a high temporal resolution of ﹩{\rm{\Delta }}t=0.1\,M﹩. Although each time step corresponds to tracking ﹩\sim {10}^{7}﹩ photons, variability on timescales shorter than ﹩\sim \mathrm{few}\,M﹩ is significantly affected by noise due to photon statistics.

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