Distributions of DM (a), burst time width (b), burst frequency width (c), Galactic Latitude b (d), and Galactic Longitude l (e). The Parkes sample (blue) consists of our 18 detections along with the 10 already discovered FRBs in this survey (Thornton et al. 2013; Champion et al. 2016; Petroff et al. 2019). For subplots (a, b), we also display, for comparison, the distribution obtained by considering the sample of the one-off FRBs published by CHIME (green, CHIME/FRB Collaboration 2021), the distribution of the sample of ASKAP one-off FRBs (orange, Shannon et al. 2018; Bannister et al. 2019; Macquart et al. 2019; Prochaska et al. 2019; Bhandari et al. 2023; Ryder et al. 2023), and the sample of FRBs detected by UTMOST (violet, Caleb et al. 2017; Farah et al. 2019; Gupta et al. 2019a,b,c, 2020a,b; Mandlik et al. 2021, 2022). For each pair of histograms in each subplot, we report the Kolmogorov-Smirnov probability p_KS of being drawn from the same distribution. Panel (f) shows the distribution of the newly detected burst arrival times in AEST local time.