Figure 2 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.

Caption: Figure 2.

1/ e falling time in the galaxy frame vs. observing energy (GeV) for MT seed photons (red) and BLR seed photons (blue).