  The K2 mission of the Kepler Space Telescope offers a unique possibility to
examine sources of both Galactic and Extra-galactic origin with high cadence
photometry. Alongside the multitude of supernovae and quasars detected within
targeted galaxies, it is likely that Kepler has serendipitously observed many
transients throughout K2. Such events will likely have occurred in background
pixels, coincidentally surrounding science targets. Analysing the background
pixels presents the possibility to conduct a high cadence survey with areas of
a few square degrees per campaign. We demonstrate the capacity to independently
recover key K2 transients such as KSN 2015K and SN 2018oh. With this survey, we
expect to detect numerous transients and determine the first comprehensive
rates for transients with lifetimes $\leq1$ day.
