Searching for new and exotic pulsars and utilizing them for advancing fundamental science is a top-priority science case for the SKA and its pathfinders. Motivated by this, and the long history of several generations of successful pulsar surveys in the southern skies, we have embarked on an all-sky survey project with the Murchison Widefield Array (MWA) – the Australian precursor for the low-frequency SKA (SKA-Low). This Southern-sky MWA Rapid Two-meter (SMART) survey is the first southern pulsar survey in the SKA-Low band and is unique in terms of novelty in data recording, survey design and an exclusive access to the pristine low-frequency band in the southern skies. The sky south of +30 degree in declination has been fully covered, amounting to four petabytes of data, however the compute-intensive nature of low-frequency pulsar searches necessitates processing in stages. Periodicity searches in 10% data have already led to 20 new pulsar discoveries, many of which are being followed up with Murriyang, uGMRT and MeerKAT. New discoveries include millisecond pulsars, low-luminosity steep-spectrum objects, and those showing sub-pulse drifting and nulling phenomena. I will present an overview of the project, survey design, science goals, processing, and science highlights. Efforts are under way to develop a fast-imaging capability to search for fast radio bursts. Aside from its enormous legacy value, SMART will also serve as an important reference for large surveys planned with SKA-Low.