We thank Dave Wootton of IBM Poughkeepsie for his valuable suggestions and comments during the development of this tool. This work has been supported in part through the Center for Astrophysical Thermonuclear Flashes at the University of Chicago by the U.S. Department of Energy under contract B532820. This work was also supported by the Mathematical, Information, and Computational Sciences Division subprogram of the Office of Advanced Scientific Computing Research, Office of Science, U.S. Department of Energy, under Contract W-31-109-ENG-38.