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Supernova explosions are among the most energetic phenomena in the knownuniverse. There are suggestions that cosmic rays up to EeV energies might beaccelerated in the young supernova shell on time scales of a few weeks toyears, which would lead to TeV neutrino radiation. The data taken with theAMANDA neutrino telescope in the years 2000 to 2006 is analysed with alikelihood approach in order to search for directional and temporalcoincidences between neutrino events and optically observed extra-galacticsupernovae. The supernovae were stacked in order to enhance the sensitivity. Acatalogue of relevant core-collapse supernovae has been created. This posterpresents the results from the analysis.

Search for High Energetic Neutrinos from Supernova Explosions with AMANDA