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It looks like the CHIANTI team recently released a new version:
https://www.chiantidatabase.org/chianti_database_history.html
CHIANTI version 11.0 has been released. It contains advanced models for ionization equilibrium for seven elements (C, N, O, Ne, Mg, Si, and S) that are an important advance for transition region ions. Further details can be found in Dufresne et al. (2024) and the CHIANTI documentation. The advanced models are currently only implemented in the IDL software, but Python versions are in development. CHIANTI 11 also includes updated atomic models for several ions, and an updated radiative recombination energy loss rate.
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