Salathe, M.Ribordy, M.Demiroers, L.2012-04-052012-04-052012-04-05201210.1016/j.astropartphys.2011.10.012https://infoscience.epfl.ch/handle/20.500.14299/79229WOS:000301312000001The current supernova detection technique used in IceCube relies on the sudden deviation of the summed photomultiplier noise rate from its nominal value during the neutrino burst, making IceCube a approximate to 3 Megaton effective detection volume - class supernova detector. While galactic supernovae can be resolved with this technique, the supernova neutrino emission spectrum remains unconstrained and thus presents a limited potential for the topics related to supernova core collapse models.Supernova neutrino detectionIceCubeGalactic supernova neutrino energy spectrumNeutrino BurstCoincidencePositronsElectronsSearchSignaltext::journal::journal article::research article