Fig. C.1
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Effect of accretion variability. The sub-panels display the distributions of the correlation slope, intercept, and offset as violin plots from the Monte Carlo simulations, used to assess the impact of variability on the best-fit empirical relations in Table 1. The bars and ’x’-markers overlaid on the violin plots indicate the reported slope, intercept, and offset values for each line from Table 1. The reported uncertainties incorporate the simulated ±50% variability to the measured line fluxes to account for non-contemporaneous log(Lacc) measurements.
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