Table 1:

Key properties of M 83 and NGC 1313^a.

Galaxy	Metallicity	D	Pix. scaleb	MB	MK	Morph.	Conf. reg.c	WNd	WCd	Cand. reg.e
	((O/H)+12)	(Mpc)	(pc2 pix-1)	(mag)	(mag)			WNE+WNL	WCE+WCL
M 83	9.0	4.5	5.32	-20.2	-23.7	SAB(s)c	132	232+250	28+526	89
NGC 1313	8.23	4.1	4.02	-18.9	-20.1	SB(s)d	70	29+22	34+0	12f

Notes. ^(a) Compiled from Hadfield & Crowther (2007); Hadfield et al. (2005) and NED. ^(b) In the images from ESO/MPI 2.2 m (+WFI) and VLT/FORS used in the analysis. A galaxy at z=0.01 in the SDSS 2.5 m images used by K08 would have 80² pc² pix^-1. ^(c) Confirmed regions containing one or more WR stars. ^(d) Total number of stars per subtype used in this paper. These numbers may differ slightly from those reported in the literature, for the following reasons: WN5-6 stars have been included in the WNE distribution; WO in WCE; transitional WN/WC have been included in both WN and WC. The total number of WR stars is obtained by adding their corresponding subtypes. ^(e) Candidate regions for which spectroscopy has not been conducted. ^(f) 11 of these are photometrically consistent with WN stars.