  Rotating Radio Transients (RRATs) are a class of pulsars characterized by
sporadic bursts of radio emission, which make them difficult to detect in
typical periodicity-based pulsar searches. Using newly developed
post-processing techniques for automatically identifying single bright
astrophysical pulses, such as those emitted from RRATs, we have discovered
approximately 30 new RRAT candidates in data from the Green Bank Telescope 350
MHz drift-scan survey. A total of 6 of these have already been confirmed and
the remainder look extremely promising. Here we describe these techniques and
present the most recent results on these new RRAT candidates.
