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Rotating Radio Transients (RRATs) represent a relatively new class of pulsar,primarily characterised by their sporadic bursting emission of single pulses ontime scales of minutes to hours. In addition to the difficulty involved indetecting these objects, low-frequency ($<$300 MHz) observations of RRATs aresparse, which makes understanding their broadband emission properties in thecontext of the normal pulsar population problematic. Here, we present thesimultaneous detection of RRAT J2325-0530 using the Murchison Widefield Array(154 MHz) and Parkes radio telescope (1.4 GHz). On a single-pulse basis, weproduce the first polarimetric profile of this pulsar, measure the spectralindex ($\alpha=-2.2\pm 0.1$), pulse energy distributions, and present the pulserates in the context of detections in previous epochs. We find that thedistribution of time between subsequent pulses is consistent with a Poissonprocess and find no evidence of clustering over the $\sim$1.5 hr observations.Finally, we are able to quantify the scintillation properties of RRATJ2325-0530 at 1.4 GHz, where the single pulses are modulated substantiallyacross the observing bandwidth, and show that this characterisation is feasibleeven with irregular time sampling as a consequence of the sporadic emissionbehaviour.

The emission and scintillation properties of RRAT J2325-0530 at 154 MHz and 1.4 GHz