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Fig. 2.

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Enlarged color image of Mothra’s arc and its surroundings. Colors are a combination of HST and JWST filters; F435W + F606W + F814W + F090W + F115W, F150W + F200W, and F277W + F356W + F410M + F444W for blue, green and red respectively. LS1 and three multiply lensed knots and their counterimages are labeled. No counterimage for LS1 is visible. Numerous faint, unresolved objects are marked with unlabeled magenta circles. These could be globular clusters or compact galactic remnants in the galaxy cluster. The white dashed line is the inferred position of the critical curve based on the ratio of the b–c separation (039) to the b′–c′ separation (032). The solid white curve is the expected position of the critical curve based on the lens model. The two curves are apart. The third counterimage of the galaxy identified in the new JWST images is shown in the bottom-left. Its position is RA = 64.046155, Dec = −24.0752067.

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