Peak intensities of SEPs as a function of flare intensity for ∼100 keV electrons (top panel), 1 MeV electrons (central panel) and ≥25 MeV protons (bottom panel) for well-connected (left), western (middle), and eastern (right) events. All symbols are same as in Fig. 2. CC_all and CC^∼* are the Spearman correlation coefficients along with p-value, for all the events in the scatter plot, and for the rest of events, excluding the starred points, respectively. CC^* is the Spearman correlation coefficient along with p-value considering only the starred points in the well-connected events. Error bars along the x-axis represent the uncertainty in the estimated GOES-equivalent flare intensity in case of behind the limb flares observed by Solar Orbiter/STIX.