GRB 250314A in the ’Amati diagram’: The samples of ’short’ (type I, in black) and ’long’ (type II, in blue) GRBs are taken from Lan et al. (2023). The peak energies and isotropic equivalent for the sample of GRBs above z = 6 are taken from Yasuda et al. (2017, GRB130606A, GRB 120521C, GRB 050904A, GRB140515A, GRB080913A, GRB090423A), Rossi et al. (2022, GRB 210905A), Brivio et al. (2025, GRB 240218A), Tanvir et al. (2018, GRB 120923A), Gorbovskoy et al. (2012, GRB 100905A), and Cucchiara et al. (2011, GRB 090429B). All errors are converted to a 68 % confidence level. The properties of GRB250314A (red) are deduced from the results of the joint ECLAIRs+GRM spectral analysis.