Images of the LMC N11 B O-type stars, from HST/WFPC2 in the F656N filter (Hα), except for PGMW 3120 (HST/ACS/F220W). The ULLYSES targets are identified with their respective IDs from Parker et al. (1992, PGMW #) and Evans et al. (2006, N11 #). The slits from different instruments are indicated, including their shapes, sizes, and position angles: FUSE FUV/MRDS (dashed magenta; 4 × 20 arcsec); HST COS (dashed cyan; D2.5 arcsec); HST STIS/E140M (black rectangle; 0.2 × 0.6 arcsec); STIS/E230M (yellow square; 0.2 × 0.2 arcsec); GIRAFFE (dashed blue; D1.2 arcsec); X-shooter UVB (dashed red; 0.8 × 11 arcsec); and X-shooter VIS (red; 0.7 × 11 arcsec). Isocontours of brightness are displayed (green) to check for multiple sources inside the slits. Scale and orientation are indicated.