Fig. 2.
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Multiply imaged clumps a, b, and c of system K8. The lower panels show the extended arc, with two counter images of the spiral galaxy shown in the upper panels. The two panels on the left show two RGB combinations of NIRCam images. In the right panel, we show Hα emission line flux obtained from the F200W grism spectra (see Appendix B), which was used to identify image K8a.1.
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