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