Resolving the mid-infrared cores of local Seyferts

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Table 1:

Observed properties of the sample.
$\begin{displaymath}\begin{tabular}{lccccr@{~~~}l@{~~~}r@{$\;\pm\;$}lr@{~~~}l@{~~... ...2.07$\;\pm\;$0.02 & 42.1$\;\pm\;$0.4 \\ \hline \end{tabular}\end{displaymath}$ ^d Distances in Mpc. ^* For NGC 1068, the fluxes are from high angular resolution (0 $.\!\!^{\prime\prime}$ 2-0 $.\!\!^{\prime\prime}$ 4) Keck and Subaru studies (Tomono et al. 2001; Mason et al. 2006) at slightly-differing wavelengths. All values for this source are written in italic font simply to draw attention to the fact that the observations are entirely drawn from other publications. See Appendix.

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