Fig. 2.
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Integrated S/N from pyplatefit versus effective radius divided by PSF full width at half maximum (FWHM) for the 66 isolated galaxies of our isolated galaxy sample. Galaxies for which GalPaK3D fits seem reliable are represented by blue dots. Galaxies with bad fits are represented by gray dots. Galaxies with bad GalPaK3D fits tend to have a low integrated S/N.
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