Fig. 12

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Finding chart of the all-sky diffuse emission. The western sky l = [180, 360] is shown with the eROSITA/eRASSl data in the 0.4–0.6 keV band. The eastern sky l = [0, 180] is shown with the ROSAT/RASS R4 (0.44–1.01 keV) band map. The green marks show the location of large projected structures, including known supernova remnants, the Large and Small Magellanic Clouds, and some extended clusters and galaxy superclusters. The color bar has been arbitrarily chosen to match the dynamic ranges of the maps.
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