Fig. 1.
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Size-mass relation for the extraplanar clumps of the Sparkler galaxy (Sect. 2). Clumps are shown as black empty circles, while the best-fitting line (obtained as described in Sect. 2.1) is plotted as the red solid line. The red shaded areas (from opaque to transparent red) show the 1σ, 2σ, 3σ intervals of the fit, respectively.
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