CHIANTI provides a database of atomic data that can be used to interpret the emission of spectral lines and continuua emitted from high-temperature, optically-thin astrophysical sources.
The CHIANTI project provides a suite of routines written in Interactive Data Language (IDL) to access the database and calculate various quantities for use in interpreting observed spectra or producing synthetic spectra.
This module will allow developers to perform all those operations rom Python as well.
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