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Since the 2011 VERITAS discovery of very high energy (VHE; E>100 GeV) gammarays from the Crab pulsar, there has been concerted effort by the gamma-rayastrophysics community to detect other pulsars in the VHE band in order toplace better constraints on emission models. Pulsar modelling demonstrates thatmuch of the magnetosphere is opaque to VHE photons, limiting emission regionsto the outer magnetosphere or beyond the light cylinder. The locations of 19known pulsars have been observed by VERITAS since full observations began in2007 with 11 locations having more than 20 hours of observations. Observationsof VHE emission from more sources could provide key data to help constraincurrent models of emission location and mechanisms. We present the status ofthe ongoing VERITAS program searching for pulsed emission in archival data.

Search for Pulsed Emission in Archival VERITAS Data