pahfit
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Model Decomposition for Near- to Mid-Infrared Spectroscopy of Astronomical Sources
Potentially a small in-notebook widget interface for enabling/disabling components. Maybe this widget can be used for the live updating plot too (issue #203).
Do we want to provide N templates for single stars and for stellar populations??
Add screen. Use different attenuation models for different set of features.
Look into optimize the fitting by using multi-processors.
Update fitting procedure to deal with the high number of lines in the simulated (and real?) JWST data. [e.g. first fit NIR segments individually, second fit all with fixed line/feature...
Update PDR science pack to include additional lines from simulated data of Orion. Related to (extension of) #186
train PAHFIT for PDRs to make PDR science pack based on ISO-SWS - Update continuum model - Update feature model where needed
Check ISO-SWS spectra on 2 galaxies to see which changes to model are related to high spectral R and which to the switch to PDRs.