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DISENTANGLING OVERLAPPING ASTRONOMICAL SOURCES USING SPATIAL AND SPECTRAL INFORMATION

  • Authors: David E. Jones, Vinay L. Kashyap, and David A. van Dyk

2015 The Astrophysical Journal 808 137.

  • Provider: AAS Journals

Caption: Figure 1.

Fitting gamma distributions to a counts spectrum. The histogram shows the observed spectrum of the brightest of the Chandra sources in the Orion field in Section 7.2 (from one iteration of our algorithm; see Section 4.3), and the curves show gamma model fits. The solid line (green) is the extended full model fit of the two-gamma spectral model and the dashed line (red) is the maximum likelihood fit of the one-gamma model.

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