Total X-ray emission observed by eROSITA in the eFEDS region during e0 (from top to bottom) in the 0.3–0.45 keV and the 0.45–0.7 keV and 0.7–2.3 keV bands, respectively. The contribution due to point sources has been removed through a wavelet filtering. Variations in the surface brightness, as large as a factor of ∼1.6, are observed in the 0.3–0.45 keV band, on scales of several degrees. The 0.7–2.3 keV band show few stripes induced by enhanced particle background, as discussed in Sect. 2. Equatorial coordinates are applied.