  Photometric survey data from the Kepler mission have been used to discover
and characterize thousands of transiting exoplanet and eclipsing binary (EB)
systems. These discoveries have enabled empirical studies of occurrence rates
which reveal that exoplanets are ubiquitous and found in a wide variety of
system architectures and physical compositions. Because the detection strategy
of these missions is most sensitive to short orbital periods, the vast majority
of these objects reside within 1 AU of their host star. Although other
detection techniques have successfully identified exoplanets at wider orbits
beyond the snow lines of their respective host stars (e.g., radial velocity,
microlensing, direct imaging), occurrence rates within this population remain
poorly constrained. As such, identifying long period objects (LPOs) from
archival Kepler and K2 data is valuable from both a statistical and theoretical
standpoint, particularly for massive gas giants which are thought to heavily
influence the formation and evolution dynamics of their respective systems.
Here we present a catalog of 164 single transit and eclipse candidates detected
during a comprehensive survey of all currently available K2 data.
