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Model Decomposition for Near- to Mid-Infrared Spectroscopy of Astronomical Sources

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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).

enhancement

Implement post-run “compound” plotting conveniences.

enhancement

Allow cubes as input to PAHFIT (in main repo or separate package?)

JWST

Do we want to provide N templates for single stars and for stellar populations??

enhancement

Add screen. Use different attenuation models for different set of features.

enhancement

Look into optimize the fitting by using multi-processors.

fitting

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...

fitting
PDRs
JWST

Update PDR science pack to include additional lines from simulated data of Orion. Related to (extension of) #186

science packs
PDRs
JWST

train PAHFIT for PDRs to make PDR science pack based on ISO-SWS - Update continuum model - Update feature model where needed

ISO
science packs
training
PDRs

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.

ISO
science packs
PDRs