X-ray-detected WR population in Wd1. We present the X-ray-brightest WR star from the top left panel and moving rightwards the X-ray brightness decreases. Each panel has a size of 10″ × 10″ and the colour coding is the same as in Fig. 1. The yellow regions are shown just for illustration purposes centred at the X-ray coordinates of the WR stars, while the magenta regions correspond to the extraction regions of detected sources used for photometry and spectral analysis, except for star A where a larger extraction region was used (Sec. 3.1).