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Supernova (SN) remnants are a well motivated candidate for the accelerationsites of cosmic rays with energies up to the knee (10^15 eV). It has beensuggested that also young SNe (~<1 year after the explosion) may be able toaccelerate cosmic rays to even higher energies. A smoking gun for cosmic-rayacceleration in young SNe would be the production of very-high-energy (VHE, >10GeV) gamma-ray radiation. The H.E.S.S. imaging air Cherenkov telescope array isan instrument sensitive to such radiation. In this contribution, the pointingdirections of the H.E.S.S. telescopes are compared to a recently published,extragalactic SN catalogue to identify coincidental observations. The resultsof the data analysis are discussed.

Search for VHE Gamma-Ray Emission from Young SNe with H.E.S.S