Figure 3 from grmonty: A Monte Carlo Code for Relativistic Radiative Transport

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grmonty: A Monte Carlo Code for Relativistic Radiative Transport

Authors: Joshua C. Dolence, Charles F. Gammie, Monika Mościbrodzka, and Po Kin Leung

DOLENCE et al. 2009 The Astrophysical Journal Supplement Series 184 387.

Provider: AAS Journals

Caption: Figure 3.

In the top panel, the spectrum of a synchrotron-emitting sphere with low optical depth above ~10 ⁸Hz viewed nearly perpendicular to the magnetic field from grmonty (crosses) and from a semi-analytic procedure (solid line). The bottom panel shows the fractional difference between the two results.

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