  We conduct a search for periodic emission in the very high-energy gamma-ray
band (VHE; E > 100 GeV) from a total of 13 pulsars in an archival VERITAS data
set with a total exposure of over 450 hours. The set of pulsars includes many
of the brightest young gamma-ray pulsars visible in the Northern Hemisphere.
The data analysis resulted in non-detections of pulsed VHE gamma rays from each
pulsar. 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 the
first such searches for pulsed VHE emission from each of the pulsars, and the
obtained limits constrain a possible flux component manifesting at VHEs as is
seen for the Crab pulsar.
