Table 3: Astrometry of the sub-images.
Object ${\rm A}_{1}$ ${\rm A}_{2}$ ${\rm A}_{3}$ ${\rm B}_{1}$ ${\rm B}_{2}$ ${\rm B}_{3}$
$x_{1}~(\hbox{$^{\prime\prime}$ })$a -0.81 -0.80 -0.58 1.04 1.04 1.04
$x_{2}~(\hbox{$^{\prime\prime}$ })$a 1.62 1.82 1.67 -0.28 -0.28 -0.28
Object ${\rm C}_{1}$ ${\rm C}_{2}$ ${\rm C}_{3}$ ${\rm D}_{1}$ ${\rm D}_{2}$ ${\rm D}_{3}$
$x_{1}~(\hbox{$^{\prime\prime}$ })$a 0.72 0.66 0.90 -0.34 -0.24 -0.54
$x_{2}~(\hbox{$^{\prime\prime}$ })$a -0.93 -1.10 -0.77 -0.98 -0.93 -0.88

a With respect to the galaxy center.


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