Figure 3 from A Method for Localizing Energy Dissipation in Blazars Using Fermi Variability

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A Method for Localizing Energy Dissipation in Blazars Using Fermi Variability

Authors: Amanda Dotson, Markos Georganopoulos, Demosthenes Kazanas, and Eric S. Perlman

Dotson et al. 2012 The Astrophysical Journal Letters 758 L15.

Provider: AAS Journals

Caption: Figure 3.

Light curves at 200 MeV, 2 GeV, and 20 GeV for BLR seed photons (upper panel) and MT seed photons (lower panel), normalized for a steady state L = 0 and maximum L = 1 (in arbitrary units). Times are in the galaxy frame. The dashed black line is the 1/ e decay time. Times are in the galaxy frame.

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