Transient phase space adapted from Nimmo et al. (2022) including the GPs detected in this work and their error bars, previous works on XTE J1810−197 (Caleb et al. 2022; Bause et al. 2024), and a recent work on FAST radio pulses from SGR J1935+2154 (Zhu et al. 2023). In the case of SGR 1935+2154, the vertical error bar of each pulse includes the uncertainty in the magnetar distance. The pink horizontal dotted line represents our flux completeness limit, and the vertical line our time resolution limit.