**Table 5:** Relevant spectroscopic data: aperture-corrected H $\alpha$ luminosities, rates of star formation based on H $\alpha$ , and extinction estimates from the Balmer decrement. In the fourth column we report extinction values based on photometric fits with spectral synthesis codes (see Sect. 4.1) and values of *SFR* corrected for slit-aperture and reddening (from Balmer lines when available). *SFR*s are in $M_\odot$ yr^-1.
$\begin{displaymath}\begin{tabular}{ l c r@{.}l c c r@{.}l } \hline \hline {\e... ...imes$: S73, no aperture correction performed.} \end{tabular} \end{displaymath}$

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