Figure 12 from THE ORIGIN OF THE COSMIC GAMMA-RAY BACKGROUND IN THE MeV RANGE

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THE ORIGIN OF THE COSMIC GAMMA-RAY BACKGROUND IN THE MeV RANGE

Authors: Pilar Ruiz-Lapuente, Lih-Sin The, Dieter H. Hartmann, Marco Ajello, Ramon Canal, Friedrich K. Röpke, Sebastian T. Ohlmann, and Wolfgang Hillebrandt

2016 The Astrophysical Journal 820 142.

Provider: AAS Journals

Caption: Figure 12.

Gamma-ray background using the HB2010 rates (private communication), together with their prediction (solid red line). The model used is the fully mixed W7 (W99b), but predictions for the other models are qualitatively similar. We show in red the calculations provided by HB2010. Our calculations using their rates are shown in black, and they agree with theirs.

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