A Study of the Soft X-ray Emission Lines in NGC 4151 II. The Internal
  Plasma Properties
  We showcase a tool suite that enables the fitting of soft X-ray spectra in
active galactic nuclei (AGN), without the need for specialist software,
allowing access to AGN physics for school students. While these standardised
Python tools were useful for measuring velocities (Note I), they offered
significantly fewer capabilities for radiative recombination continua (RRC),
and R and G ratios, utilised to obtain the internal plasma properties within
the out owing wind seen in NGC 4151. Although further work is required for
these tools to be used in outreach projects, we present findings of the plasma
temperature and density in NGC 4151 spanning a 15 year period.
