Table 1: Differential astrometry for HE 0047-1756, based on the GALFIT results for the i and $K_{\rm s}$ band images. Component A is the brighter of the two QSO components. The quoted error bars are only the internal errors given by the fitting routine. The last object is the faint blob southwest of component B.
\begin{displaymath}\begin{tabular}{lr@{$\;\pm\;$}lr@{$\;\pm\;$}l} \hline\hline\n... ... & $-$2.36 & 0.15 \\ \noalign{\smallskip }\hline \end{tabular}\end{displaymath}


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