Fig. A.1

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Star cluster surface density profile around GAMA 526784 from galaxy centre in terms of Re. The blue scatter points and error bars are the measurements. The black curve is the Sérsic model fit to the total star cluster distribution. The dash-dotted grey line is the number density contribution of the background measured outside of 5 Re. This number density profile is calculated before selecting the clusters within 3 Re of GAMA 526784.
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