Reconstruction results from the eROSITA early data release (EDR) observation of SN1987A in the LMC. Top row (left to right): exposure- and effective-area-corrected observed data, reconstructed extended emission associated with 30 Doradus C, and reconstructed extended emission from the Tarantula Nebula. Bottom row (left to right): reconstructed total sky signal (including all modeled components), reconstructed diffuse background emission (excluding point and extended sources), and reconstructed point-source emission field. The point source field has been convolved with a Gaussian kernel with a standard deviation of 4″. All panels employ the same RGB color scheme, representing intensities in the three energy bands: red (ν_low = 0.2–1.0 keV), green (ν_ref = 1.0–2.0 keV), and blue (ν_hi = 2.0–4.5 keV).