All Tables

Table 1: Fluxes of selected regions in the ultraviolet, H $\alpha$ , and mid-infrared (3.6, 4.5, and 8.0 $\mu$ m). The "-'' symbol indicates that the region falls outside the field of view, " $\le$ '' means the aperture is heavily polluted by stars and the flux is therefore likely being overestimated and " $\ge$ '' means the aperture does not contain all of the object, e.g., to avoid a foreground object, the actual flux then being underestimated.
Table 2: Star formation rates deduced from the ultraviolet, H $\alpha$ , and mid infrared, in solar mass per year. The symbol ":'' means the estimation is uncertain.
Table 3: Mean flux and SFR ratios for the different samples. Extremely discrepant points (if any) have been discarded before performing the calculation.