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We conduct a search for periodic emission in the very high-energy gamma-rayband (VHE; E > 100 GeV) from a total of 13 pulsars in an archival VERITAS dataset with a total exposure of over 450 hours. The set of pulsars includes manyof the brightest young gamma-ray pulsars visible in the Northern Hemisphere.The data analysis resulted in non-detections of pulsed VHE gamma rays from eachpulsar. Upper limits on a potential VHE gamma-ray flux are derived at the 95%confidence level above three energy thresholds using two methods. These are thefirst such searches for pulsed VHE emission from each of the pulsars, and theobtained limits constrain a possible flux component manifesting at VHEs as isseen for the Crab pulsar.

A Search for Pulsed Very High-Energy Gamma Rays from Thirteen Young Pulsars in Archival VERITAS Data