Figure 14 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 14.

Top panel shows the spectrum of a snapshot from a HARM simulation of a turbulent accretion flow onto a Kerr black hole as computed by ibothros (solid line) and grmonty (crosses). Bottom panel shows the fractional difference between the two.

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