Radio power versus mass diagrams (150 MHz, left column; 1.4 GHz, right column). Small shaded circles are from the literature at lower-redshifts (Di Gennaro et al. 2021a; Botteon et al. 2022), while stars display the detection from the MaDCoWS clusters in LoTSS-DR2 presented in this work. All markers are colour-coded according to their redshifts. We also display the P_ν − M₅₀₀ correlations found by Cuciti et al. (2023) and Cassano et al. (2013), at 150 MHz (left panels) and 1.4 GHz (right panles) respectively. Top row: masses from CARMA 30 GHz observations (Decker et al. 2019). Middle row: masses from the richness-mass scale relation calibrated with ACT clusters (Orlowski-Scherer et al. 2021, OS+21); solid errorbars reflect the uncertainties on the slope of the scale relation, while the dashed errorbars define the uncertainties associated with the scatter of the scale relation. Bottom row: masses from eROSITA observation.