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Fig. 11
AIRX vs. β for IR-detected galaxies in the UV sample. Top: β is measured from the spectra. The black line is a fit to the data (Eq. (6)). Bottom: β is measured from photometry. The red line is a fit to the data (Eq. (7)). The black line is the relation for βspec.
This figure is made of several images, please see below:
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