  The Kilodegree Extremely Little Telescope (KELT) survey is a ground-based
program designed to search for transiting exoplanets orbiting relatively bright
stars. To achieve this, the KELT Science Team operates two planets facilities -
KELT-North, at Winer Observatory, Arizona, and KELT-South, at the South African
Astronomical Observatory. The telescopes used at these observatories have
particularly wide fields of view, allowing KELT to study a large number of
potential exoplanet host stars. One of the major advantages of targeting bright
stars is that the exoplanet candidates detected can be easily followed up by
small, ground-based observatories distributed around the world. This paper will
provide a brief overview of the KELT-North and the KELT-South surveys, the
follow-up observations preformed by the KELT Follow-up Collaboration, and
exoplanet discoveries confirmed thus far, before concluding with a brief
discussion of the future for the KELT program.
