I know you have options to overplot spectral line labels from querying ADAS and NIST, so I was wondering about allowing to give data from other atomic data sources.
I'm particularly thinking from FAC, SCRAM, or FLYCHK. All have different output format so maybe it's on the user to read the files. But from these you could overplot things like the A-values at a transition wavelength, or the PEC [cm^3/s] -slash- emissivity [ph/cm3/s] at a transition wavelength, or even a spectral emissivity [ph/cm3/s/AA] convoluted (maybe by user?) with some line shape over a wavelength vector
atomdb and Chianti also have similar line labeling overplots, but are more optimized for the astrophysical community so carry data for Z<=30
I'm also aware of a stash of such data curated by General Atomic folks that they also use to do similar line identification in their spectra
I know you have options to overplot spectral line labels from querying ADAS and NIST, so I was wondering about allowing to give data from other atomic data sources.
I'm particularly thinking from FAC, SCRAM, or FLYCHK. All have different output format so maybe it's on the user to read the files. But from these you could overplot things like the A-values at a transition wavelength, or the PEC [cm^3/s] -slash- emissivity [ph/cm3/s] at a transition wavelength, or even a spectral emissivity [ph/cm3/s/AA] convoluted (maybe by user?) with some line shape over a wavelength vector
atomdb and Chianti also have similar line labeling overplots, but are more optimized for the astrophysical community so carry data for Z<=30
I'm also aware of a stash of such data curated by General Atomic folks that they also use to do similar line identification in their spectra