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The advent of gravitational wave and neutrino astronomy has led to an exciting era of multi-messenger astronomy. Identifying high-energy neutrino emission from compact binary mergers could shed light on the sources of high-energy neutrino emission as well as particle acceleration mechanisms in these compact binary systems. The LIGO-Virgo Collaboration (LVC) has reported 65 compact binary merger candidates as of March 5th, 2020. We present a search for high-energy neutrino emission from each merger reported by LVC using the IceCube neutrino observatory.