Top: X-ray bolometric luminosity–mass relation for the weak-lensing peaks in the eFEDS footprint. Blue circles show the shear-selected clusters with a unique eFEDS match; orange diamonds display weak-lensing peaks with a primary eFEDS counterpart; and red squares show weak-lensing clusters with no eFEDS match. eFEDS clusters are displayed as light purple asterisks and its corresponding fit is given by the black solid line. For comparison, the data of the X-ray selected clusters presented in Mahdavi et al. (2013, grey pentagons), and the shear-selected clusters studied in Giles et al. (2015, green pentagons) are plotted. The fit to the shear-selected cluster is given by the dashed-red line, and for two sub-samples of them the fits are shown by the dotted-green and dashed-dotted blue lines. Bottom: ratio of the different normalisations of the distinct shear-selected cluster to normalisation of the eFEDS clusters fit.