Fig. 6.
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Mean light-weighted IR correction factors, ⟨kIR⟩IR as a function of the aperture and the inclination using the galaxies in the Auriga-D sample. The aperture is given as a fraction of the optical radius, with the gray region denoting a median aperture of 15−20 kpc of the simulated galaxies. The values from B16 are shown as gray lines.
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