  The advent of Multi-Messenger Astronomy has allowed for new types of source
searches within the neutrino community. We present the results of the first
search for GeV astrophysical neutrinos emitted from Compact Binary Mergers,
i.e. binary black hole or binary neutron star mergers, detected by the LIGO and
Virgo interferometers. We introduce a new approach that lowers the energy
threshold of IceCube from roughly 10 GeV to <1 GeV. This method uses an
innovative event selection of GeV neutrino events in IceCube and searches for a
statistically significant increase in the amount of GeV-like events detected
around the Compact Binary Merger time. We compare our results with constraints
set by high-energy neutrino searches, and describe the complementarity of these
low and high-energy searches.
