This proposal concentrates the timing observations of binary and millisecond pulsars discovered by us in the Parkes Multibeam (PKSMB) and high-latitude (PH) surveys. In order to fully exploit the s
Fast radio bursts (FRBs) continue to raise more questions than they answer. Until last year, only one burst – the only one known to repeat - had been localized to a bright radio nebula (either a young
