telescopes, the Murchison Widefield Array has enormous potential to
conduct blind searches for radio transients and probe the nearby
pulsar population. We are working to develop a common framework
with the Australian Square Kilometer Array Pathfinder (ASKAP)
Variables and Slow Transients (VAST) survey to allow real-time
transient detection and characterization. I will discuss the expected
types of sources that we hope to discover with the full array and
review some of the initial results from our 32-element testbed.