The Galaxy Cluster 'Pypeline' for X-ray Temperature Maps: ClusterPyXT
  ClusterPyXT is a new software pipeline to generate spectral temperature,
X-ray surface brightness, pressure, and density maps from X-ray observations of
galaxy clusters. These data products help elucidate the physics of processes
occurring within clusters of galaxies, including turbulence, shock fronts,
nonthermal phenomena, and the overall dynamics of cluster mergers. ClusterPyXT
automates the creation of these data products with minimal user interaction,
and allows for rapid analyses of archival data with user defined parameters and
the ability to straightforwardly incorporate additional observations. In this
paper, we describe in detail the use of this code and release it as an open
source Python project on GitHub.
