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# Support for tabulated Atomic Spectra
Major project: it would require some new features:
- [ ] support Atomic Line database Imports (NIST/Chianti), convert to the known Pandas format to use th…
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reported by: @CloudyLex
They have a new version with changed format. It will be easier to expand our stout database than have to deal with these changes.
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From: Giulio Del Zanna
Subject: CHIANT…
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While some parts of the fiasco database are specific to CHIANTI, the overall package structure would be well suited to interface with other atomic databases as well, e.g.
* [AtomDB](http://www.atom…
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Version 9.0 of the [Chianti database](https://www.chiantidatabase.org/) has some notable changes:
> With Version 9.0, CHIANTI explicitly includes the processes of dielectronic recombination and aut…
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Following up on #16, it'd be helpful to document the steps necessary to create the HDF5 file from the ionization and recombination rates. While doing this, we should also document what the structure …
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This is a very interesting project! Much of my research (coronal loop physics) involves calculating NEI states for impulsively heated loops so I was excited to find another Python project with this sa…
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What sorts of tools and collaborations can we leverage to minimize unnecessary reproduction of effort?
Here are some that were mentioned in PlasmaPy/PlasmaPy#162 :
* [MassiveOES](https://bitbucket…
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# Molecular databases
### Exomol
See initial work in https://github.com/keflavich/Orion_ALMA_2016.1.00165.S/blob/master/analysis/parse_exomol_files.py
- See also: https://github.com/xnx/ExoM…
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As mentioned by @wtbarnes in #11 , we should properly define the scope of the project.
My current thinking is that the project should cover (copypasta from the current README):
* Creating a genera…
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reported by: @CloudyLex
There can be more than one type of radiative transition between some levels - an example being the 2s-1s transition in H-like species. Currently we stop when more than one t…