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We report on the analysis of 13 gamma-ray pulsars discovered in theEinstein@Home blind search survey using Fermi Large Area Telescope (LAT) Pass 8data. The 13 new gamma-ray pulsars were discovered by searching 118unassociated LAT sources from the third LAT source catalog (3FGL), selectedusing the Gaussian Mixture Model (GMM) machine learning algorithm on the basisof their gamma-ray emission properties being suggestive of pulsarmagnetospheric emission. The new gamma-ray pulsars have pulse profiles andspectral properties similar to those of previously-detected young gamma-raypulsars. Follow-up radio observations have revealed faint radio pulsations fromtwo of the newly-discovered pulsars, and enabled us to derive upper limits onthe radio emission from the others, demonstrating that they are likelyradio-quiet gamma-ray pulsars. We also present results from modeling thegamma-ray pulse profiles and radio profiles, if available, using differentgeometric emission models of pulsars. The high discovery rate of this survey,despite the increasing difficulty of blind pulsar searches in gamma rays,suggests that new systematic surveys such as presented in this article shouldbe continued when new LAT source catalogs become available.

The Einstein@Home Gamma-Ray Pulsar Survey II. Source Selection, Spectral Analysis and Multi-wavelength Follow-up