Fig. 1.
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Archival HST/WFC3 F110W negative image of the PLCK G165.7+67.0 field (1′×0.7′). The triply imaged arcs 2a, 2b, and 2c of the SN H0pe host galaxy are highlighted with magenta circles with a radius of 1″ (credits: Frye et al. 2019). The highlighted regions are part of an arc produced by strong lensing from the foreground galaxy cluster.
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