Table 3: Table for derived quantities for the different regions. The last row gives the mean and standard deviation for all the regions. Column 2 is the SFR derived from the observed H$\alpha $ flux, and Col. 3 corrects the SFR for the extinction given in Table 2. Column 4 gives the best fit age. The mass (Col. 5) is determined from population modelling. The mass to light ratio (Col. 6) uses the luminosity LB derived from the B magnitude relative to the AB magnitude for the sun $M_{B,{\odot }}=5.33$. Column 7 lists the specific SFR per Gyr normalised to the mass after correction for the host extinction, and Col. 8 lists the luminosity specific SFR, both derived after correcting for intrinsic extinction.
\begin{displaymath}\begin{tabular}{l r@{.}l r@{.}l r r@{.}l r@{.}l r@{.}l r@{.}l... ...\pm$~0.04 & 38&~$\pm$~42 & 38&~$\pm$~52\\ \hline \end{tabular}\end{displaymath}


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