Fig. 11.
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Accuracy of the attenuation correction scheme of Tully & Fouqué (1985) and Tully et al. (1996). The three panels correspond to three different broadbands: GALEX NUV, SDSS r, and 2MASS H. Pink dots compare the intrinsic to the dust-attenuated absolute magnitudes for the galaxies in our TNG50 sample. Chocolate dots compare the intrinsic to the attenuation-corrected absolute magnitudes.
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