A new iterative fitting routine deblends unresolved AGN emission from resolved host-galaxy emission in IFS datacubes by jointly modeling a Moffat PSF and a Sérsic host profile per wavelength slice.
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An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations
A new iterative fitting routine deblends unresolved AGN emission from resolved host-galaxy emission in IFS datacubes by jointly modeling a Moffat PSF and a Sérsic host profile per wavelength slice.