pahfit
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PAHFIT
Model Decomposition for Near- to Mid-Infrared Spectroscopy of Astronomical Sources
Should add the units to the model pack and output files. This would require the ingest of the model pack to make sure to convert the units to the internally...
Would be good to couple the data to an instrument pack. Not quite sure how to do this, but this would make it clear the coupling of the instrument pack...
Later versions of IDL PAHFIT (never widely released) toyed with allowing redshift `z` to be a free parameter. It wasn't widely tested and worked poorly. Free redshift obviously introduces some...
We need a simple and flexible means of expressing constraints on _and between_ parameters, for the input specification discussed in #9. Examples that can be attached to one parameter: 1....
It's very common now to PAHFIT hundreds or more spectra over and over, from large samples to spectral cubes. This can get slow. Optimizers usually run on one processor. I...
Here is the next pull request. I have just rebased this branch on dev. Replaces #225 , and this should be the final part of #280 . Changes with respect...
Currently, `tau` is used as the strength of the blackbody (stellar continuum) and modified Blackbody (dust continuum) components, and the equation for evaluating the blackbody looks like this ``` amplitude...
In my recent work, I have started a new habit where I treat science packs in a modular way. An example use cases is as follows: You have two objects:...
Both intensity (e.g. `MJy/sr`) and flux (e.g. `mJy`) unit flavors are prevalent among the spectra PAHFIT encounters. To simplify unit conversion and support a variety of spectral input units, we...