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The most numerous source class that emerged from the H.E.S.S. Galactic PlaneSurvey are Pulsar Wind Nebulae (PWNe). The 2013 reanalysis of this survey,undertaken after almost 10 years of observations, provides us with the mostsensitive and most complete census of gamma-ray PWNe to date. In addition to auniform analysis of spectral and morphological parameters, for the first timealso flux upper limits for energetic young pulsars were extracted from thedata. We present a discussion of the correlation between energetic pulsars andTeV objects, and their respective properties. We will put the results incontext with the current theoretical understanding of PWNe and evaluate theplausibility of previously non-established PWN candidates.

A Population of Teraelectronvolt Pulsar Wind Nebulae in the H.E.S.S. Galactic Plane Survey