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Fig. 1.

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Total X-ray emission observed by eROSITA in the eFEDS region, during e0. The contribution due to point sources has been removed through a wavelet filtering. In red, green, and blue colours we show the 0.3–0.45 keV; 0.45–0.7 keV, and 0.7–2.3 keV bands, respectively. Variations of the surface brightness of the diffuse emission are clearly observed from a sub-degree to several degrees scale. The brightest patch appears slightly redder, which is consistent with the inference that the flux in the soft band is less absorbed. Equatorial coordinates are applied.

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