**Table 5:** The properties of the massive star clusters.
Name	M_V^a	$R_{\rm eff}$	$\sigma$	age	Mass
	(mag)	(pc)	(km s^-1)	Gyr	( $10^{7}~{\cal{M}}_{\odot}$ )
NGC 7252:W3	-16.2	$17.5\pm1.8$	$45\pm5$	$0.4\pm0.15$	$8\pm2$
NGC 7252:W30	-14.6	$9.3\pm1.7$	$27.5\pm2.5$	$0.4\pm0.15$	$1.59\pm0.26$
NGC 1316:G114	-13.0	$4.08\pm0.55$	$42.1\pm2.8$	$3\pm1$	$1.64\pm0.13$

^a We have corrected for foreground extinction of NGC 7252 and NGC 1316 of A_V = 0.03 and A_V = 0.0 respectively.

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