Fig. 18 from Inferring the Spatial and Energy Distribution of Gamma‐Ray Burst Sources. III. Anisotropic Models

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Inferring the Spatial and Energy Distribution of Gamma‐Ray Burst Sources. III. Anisotropic Models

Authors: Thomas J. Loredo and Ira M. Wasserman

Loredo & Wasserman 1998 The Astrophysical Journal 502 108.

Provider: AAS Journals

Caption: Fig. 18.

Predicted peak flux distribution for the best‐fit ν_h = 1.5 two‐population model for the 1024 ms data. (a) Predicted (smooth curve) and observed (histogram) cumulative intensity distributions. (b) Total differential rate (solid line), with halo (dashed line) and cosmological (dotted line) components plotted separately.

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