Analysis of galaxy spectral energy distributions from far-UV to far-IR with CIGALE: studying a SINGS test sample

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Table 2:

Properties of the SINGS test sample.
$\begin{displaymath}\begin{tabular}{l l r@{.}l r@{\ $\pm$\ }l r@{\ $\pm$\ }l r@{\... ...04 & 2.66 & 0.50 \\ \noalign{\smallskip } \hline \end{tabular}\end{displaymath}$ Although we list the relatively conservative run B results (see Sect. 3.2.2), the given standard deviations could underestimate the real uncertainties because of the limited model grid used, model inaccuracies, and possible unconsidered photometric errors. ^a See Kennicutt et al. (2003); ^b significant deviations of the metallicity from the solar value may affect the results for $t_{{\rm D4000}}$ (see Sect. 3.2.1).

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