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Fig. 9.

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X-ray luminosity within 300 kpc, without masking extended X-ray sources, for quiescent (top left) and star-forming (bottom left) central galaxies, and central and satellite galaxies together, compared to Comparat et al. (2022). Also shown are the satellite fractions to explain the bright LX of quiescent galaxies Comparat et al. (2022). X-ray luminosity within 10–100 kpc, after masking all X-ray sources and subtracting XRB emission, for quiescent (top right) and star-forming (bottom right) central galaxies, central and satellite galaxies together, compared to Chadayammuri et al. (2022). Also shown is the LX, CGM of central star-forming galaxies selected in eFEDS sky area and galaxies with star companion.

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