Parkes observations for project P786 semester 2012APRS

Rotating Radio Transients (RRATs), neutron stars from which sporadic radio bursts are detected, represent approximately 3% (and increasing) of radio-emitting pulsars as they are found via single-pulse searches of archival and current pulsar surveys. Their sporadic emission makes them difficult to study and nearly all information about the properties of the objects is the result of dedicated monitoring and timing programs at Parkes telescope. This project represents the largest (and most successful) effort in constraining RRAT properties and origins. Through RRAT monitoring and timing, we will continue to determine basic RRAT properties. This will enable us to identify physical causes for the extreme RRAT emission, deduce how RRATs are related to the general pulsar and magnetar populations, and explore the distribution of extreme radio intermittence in neutron stars.