A major breakthrough in fast radio burst (FRB) astronomy was recently made when the repeating FRB 121102 was localized to sub-arcsecond precision. The bursts were found to originate in a bright radio
We propose to carry out fortnightly monitoring of a very active repeater, FRB~190520, with the Parkes UWL system. Our current observations show that FRB~190520 is not only the most active FRB that can
Observationally, there are two basic types of Fast Radio Bursts (FRBs): repeating and non-repeating ones. In the southern sky, there are very limited number of repeaters we can monitor unless more are
