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The era of multimessenger astrophysics has arrived with the simultaneousoperation of large cosmic-ray, gamma-ray, neutrino, and gravitational-waveobservatories. In just the past two years, an electromagnetic (EM) counterpartwas detected for a gravitational wave event, and evidence for an EM counterpartof high energy neutrinos has been identified. These measurements have had amajor impact on our view of the non-thermal universe, but understanding cosmicaccelerators require a substantial increase in the number of multimessengerobservations. The Astrophysical Multimessenger Observatory Network (AMON) isdesigned for high-statistics searches of sub-threshold transient alerts fromgamma-ray and neutrino detectors. Within AMON, we have implemented ajoint-likelihood analysis of TeV gamma-ray measurements from the High AltitudeWater Cherenkov (HAWC) Observatory and neutrinos from the IceCube NeutrinoObservatory. AMON is ready to produce real-time coincidence alerts using HAWC"hotspots" and IceCube astrophysical neutrino events. These alerts will bedistributed to AMON follow-up partners with a median anticipated delay of sixhours, which corresponds to a full transit in the field of view of HAWC. Thealerts will have an angular resolution of ${\sim}0.2^{\circ}$, making themwell-suited for deep electromagnetic follow-up observations.

AMON: TeV Gamma and Neutrino Coincidence Alerts from HAWC and IceCube subthreshold data