Table 2: The selection of the sample of stellar cluster candidates with accurate radii. The numbers indicate the amount of sources that satisfy the mentioned criterion and all the criteria mentioned above it, split in the low, intermediate and high background region.
Criterion Nr. remaining

low inter high

All sources 35 980 15 809 23 647

$\mbox{$R_{\rm eff}$ }> 0.5$ pc 11 064 4799 7238

$\chi^{2}/\chi_{0}^{2} < 1$ 10 715 4661 7028

${\it F435W}< 22.5$ mag

${\it F555W}<22.3$ mag 472 346 1301

${\it F814W}<22.7$ mag

$\vert R_{{\it F435W}}-R_{{\it F555W}}\vert < 2$ pc 457 327 1068

No neighbour within 5 pixels 418 302 939

After visual inspection 317 239 728

Total sample: 1284

**Table 2:** The selection of the sample of stellar cluster candidates with accurate radii. The numbers indicate the amount of sources that satisfy the mentioned criterion and all the criteria mentioned above it, split in the low, intermediate and high background region.
Criterion		Nr. remaining
	low	inter	high
All sources	35 980	15 809	23 647
$\mbox{$R_{\rm eff}$ }> 0.5$ pc	11 064	4799	7238
$\chi^{2}/\chi_{0}^{2} < 1$	10 715	4661	7028
${\it F435W}< 22.5$ mag
${\it F555W}<22.3$ mag	472	346	1301
${\it F814W}<22.7$ mag
$\vert R_{{\it F435W}}-R_{{\it F555W}}\vert < 2$ pc	457	327	1068
No neighbour within 5 pixels	418	302	939
After visual inspection	317	239	728
Total sample: 1284

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