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  • I implemented the photon and energy flux and error calculations that Jean requested and that were described in my talk at the Monday session of the Collaboration meeting. This is in Likelihood v13r18, pyLikelihood v1r6, and ST HEAD1.686. There is documentation on confluence
  • For the DM group, I have implemented a class that will handle multiple likelihood analyses for different regions of the sky simultaneously, tying together the spectral parameters that are expected to be same, i.e., the parameters describing with the dark matter spectrum. The basic idea was outlined by Jan Conrad during the DM splinter meeting. This is in Likelihood v13r18p3, pyLikelihood v1r7, and ST LATEST1.2465

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