  The K2 mission is a repurposed use of the Kepler spacecraft to perform
high-precision photometry of selected fields in the ecliptic. We have developed
an aperture photometry pipeline for K2 data which performs dynamic automated
aperture mask selection, background estimation and subtraction, and positional
decorrelation to minimize the effects of spacecraft pointing jitter. We also
identify secondary targets in the K2 "postage stamps" and produce light curves
for those targets as well. Pipeline results will be made available to the
community. Here we describe our pipeline and the photometric precision we are
capable of achieving with K2, and illustrate its utility with asteroseismic
results from the serendipitous secondary targets.
