Image Details
Caption: Figure 16.
Global SFRs derived from the WISE 12, 22 μm and GALEX FUV and NUV luminosities, compared to the neutral hydrogen content (see Table 6 for details). For comparison, also shown are the SFRs that follow from the Donoso et al. (2012) 12 μm relations of starburst, intermediate, and AGN galaxy types. The dashed line corresponds to the trend observed in the SINGS sample (Cluver et al. 2010).
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