Location of GRB 200716 (red star) in the rest-frame (E_iso, E_p, z) plane for the short-duration GRBs (grey squares) and the long-duration GRBs (black circles) of Tsvetkova et al. (2017). The grey solid line indicates the Amati relation estimated using the long-duration GRBs of Tsvetkova et al. (2017), while the grey dashed lines indicate its 3σ uncertainty. The orange dotted line shows the position of the burst for 0.341 ≤ z ≤ 10.