Comments (3)
Shifting spectra in wavelength changes integrated feature strength (in the same way as redshift) and wouldn't work for smooth functions like blackbodies. Is there any reason we can't just fit a suite of parallel models with absolute ties between the "same" lines/features (in terms of integrated strength)? The modeler doesn't care about "wavelength" after all. Not sure how continuum would get treated (we need to demand it is "continuous" and identical in the overlap regions).
This would definitely stress the parameter constraint apparatus of the model framework. This is a long range enhancement I'd guess. It definitely relates closely to the issue of spectral stitching discussed in #16. How much of this is PAHFIT's job? Reasonable people can disagree.
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I agree with all your comments. :-)
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This old issue leads to AstroPy's JointFitter and related "fit overlapping spectra in parallel" ideas. Currently not implemented given the limitations of the joint fitter, but part of the new model plan.
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Related Issues (20)
- Update automated services HOT 4
- Can't import pahfit since astropy 6.0.0 HOT 3
- Readthedocs build failing HOT 1
- Feature for trivial or custom instrument pack HOT 2
- Obscure bug in Features table formatter HOT 5
- features.util.bounded_is_fixed() does not work for dust_feature-only science packs HOT 5
- Unit of the output power and HOT 1
- Where to host notebooks? HOT 6
- Use of pkg_resources HOT 1
- Wavelength range for MIRI instrument packs
- Piecewise/partial integration of drvdputt/experimental HOT 7
- Use QTable instead of Table HOT 1
- features.loc[feature_name] not working consistently HOT 1
- Allow `Fitter` reuse in `Model` HOT 1
- Implement Sara Profile (Drude convolution) HOT 1
- Always use / for PosixPath
- Joint/Multi-Fit in the Model<->Fitter paradigm HOT 1
- Sara Profile Analytic (or semi-analytic) version
- Introduce sigma_v + v_off, and remove line FWHM as a user-settable parameter HOT 2
- flux density shift to rest frame is not correct HOT 6
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