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In June 2019 the Earth will approach within 5{\deg} mean anomaly of thecentre of the Taurid resonant swarm, its closest post-perihelion encounter withEarth since 1975. This will be the best viewing geometry to detect and placelimits on the number of NEOs proposed to reside at the swarm centre until theearly 2030s. We present an analysis of the optimal times and pointing locationsto image NEOs associated with the swarm

The 2019 Taurid resonant swarm: prospects for ground detection of small NEOs