Fig. 11.

Download original image
Stacked difference , where αi was chosen to minimize the contribution from the arc to the difference, and FnnnWi are all filters with wavelengths below 2 μm, that is F090W, F115W, and F150W. These were degraded to the resolution of F200W using the star-derived PSF in Appendix B. The individual differences are shown in Col. 3 of Fig. B.2. The stacked image has been smoothed with a Gaussian of
to increase the contrast. The position of LS1 is marked with a white arrow. The position of the possible counterimage LS1′, ≈0
1 from LS1, is marked with a yellow circle.
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