LMC mosaic from eROSITA observations around SN 1987A and N 132D. Red, green, and blue represent X-ray energies in the bands 0.2–1.0keV, 1.0–2.0keV, and 2.0–4.5keV, respectively. The HMXB pulsars are marked with white circles and labelled with their pulse period measured near the time of their discovery. HMXBs and candidates without known pulse period are indicated by green circles and the entry number from Table 2.