Table 1: Estimated star cluster surface densities at different elliptical annuli from sample in B filter.
Range (pix) NPTS NPTS_w $\rho_0$ (kpc^-2) $N_{\rm GC}$ (range) $N_{\rm GC}$ (cum.)

0-100 * * 1.59 $\pm$ 0.40 253.5 $\pm$ 63.8 253.5 $\pm$ 63.8

100-200 36 85.4 0.82 $\pm$ 0.21 392.2 $\pm$ 100.4 645.7 $\pm$ 164.2

200-350 121 267.2 0.60 $\pm$ 0.09 789.2 $\pm$ 118.4 1434.9 $\pm$ 282.6

350-500 175 378.5 0.38 $\pm$ 0.05 772.5 $\pm$ 101.6 2207.4 $\pm$ 384.2

500-800 413 761.2 0.08 $\pm$ 0.02 497.4 $\pm$ 124.4 2704.8 $\pm$ 508.6

Column 1: range in pixels between inner and outer semi-major axes of annulus used for source counts (1 kpc = 21 pixels); Col. 2: total number of sources found in the annulus; Col. 3: total weighted number of sources in annulus; Col. 4: normalization density of Gaussian fit to GCLF at given annulus, as explained in text (in units of kpc^-2); total expected number of clusters in annulus, obtained as explained in the text.

**Table 1:** Estimated star cluster surface densities at different elliptical annuli from sample in B filter.
Range (pix)	NPTS	NPTS_w	$\rho_0$ (kpc^-2)	$N_{\rm GC}$ (range)	$N_{\rm GC}$ (cum.)
0-100	*	*	1.59 $\pm$ 0.40	253.5 $\pm$ 63.8	253.5 $\pm$ 63.8
100-200	36	85.4	0.82 $\pm$ 0.21	392.2 $\pm$ 100.4	645.7 $\pm$ 164.2
200-350	121	267.2	0.60 $\pm$ 0.09	789.2 $\pm$ 118.4	1434.9 $\pm$ 282.6
350-500	175	378.5	0.38 $\pm$ 0.05	772.5 $\pm$ 101.6	2207.4 $\pm$ 384.2
500-800	413	761.2	0.08 $\pm$ 0.02	497.4 $\pm$ 124.4	2704.8 $\pm$ 508.6

Source LaTeX | All tables | In the text