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It is anticipated that the forthcoming Cherenkov Telescope Array (CTA) willinclude a number of medium-sized telescopes that are constructed using adual-mirror Schwarzschild-Couder configuration. These telescopes will sample awide ($8^{\circ}$) field of view using a densely pixelated camera comprisingover $10^{4}$ individual readout channels. A readout frequency congruent withthe expected single-telescope trigger rates would result in substantial datarates. To ameliorate these data rates, a novel, hardware-level DistributedIntelligent Array Trigger (DIAT) is envisioned. A copy of the DIAT operatesautonomously at each telescope and uses reduced metadata from a limited subsetof nearby telescopes to veto events prior to camera readout. We present theresults of Monte-Carlo simulations that evaluate the efficacy of a "Parallaxwidth" discriminator that can be used by the DIAT to efficiently distinguishbetween genuine gamma-ray initiated events and unwanted background events thatare initiated by hadronic cosmic rays.

Simulations of a Distributed Intelligent Array Trigger for the Cherenkov Telescope Array