ChiantiPy version 0.15.0
from the changelog
Significant improvement have been made. It is now possible to calculate spectral line intensities in wavelength/energy units of angstroms, nm, eV, or keV
Calculations of the continuum still require that the wavelengths are in angstroms.
The free-bound continuum now includes the photoionization cross sections of Verner for recombination to the ground level
The free-free continuum has been correction to use the ion charge, not the nuclear charge previously used
A new class MradLoss.mradLoss has been created. It allows multiprocessing calculations of the radiative loss rate
The chiantirc file can now also be placed in the $HOME/.config directory