Table 2:

Fractional fluxes at the locations of the WR stars^a.

	IDb	Subtypec	Number	FFd
	1	WNL	3	0.29
	2	WCL	2	0.34
	3	WCL	2	0.26
M 83	4	WNE	16	0.48
	5	WCL	8	0.48
	6	WCE	3	0.06
	...	...	...	...
	133	cand.	...	0.25
	134	cand.	...	0.54
	1	WNE	1	0.37
	2	WCE	1	0.30
NGC 1313	3	WNL	1	0.06
	...	...	...	...
	28	cand.	...	0.38

Notes. ^(a) An indicative portion of this table is shown. For the full table refer to the electronic version of the Journal. ^(b) We follow the exact numbering of Hadfield et al. (2005) and Hadfield & Crowther (2007). Additional info (e.g. fluxes, errors in star numbers) can be found in these references. ^(c) ``cand''. stands for candidate region. ^(d) These fractional fluxes refer to a binning of 15 and 19 for the images of M 83 and NGC 1313 we have used, respectively. Although we have shown that the results do not change significantly with the choice of binning, individual fractional fluxes can vary.