In pulsar moded events are screened correctly for zenith angle and TASC minimum energy. There are small changes in the various data displays. The results of fitting are put into a FITS format file. The program now works with the new-format timeline file. Graphs can now be produced for broken power law models.
Minor bug fixes.
There are now two different modes of operation. The program can do pulse-phase spectroscopy of a pulsar or it can analyze a DC source. In the latter case, the data comes from a likelihood analysis. The diffuse background model has been removed. It is no longer needed.