Fitoussi, C.; Raisbeck, G.M.; Knie, K.; Korschinek, Gunther; Faestermann, T.; Goriely, S; Lunney, D.; Poutivtsev, M.; Rugel, G.; Waelbroeck, Claire; Wallner, Anton
An Fe60 peak in a deep-sea FeMn crust has been interpreted as due to the signature left by the ejecta of a supernova explosion close to the solar system 2.8±0.4Myr ago. In an attempt to confirm this interpretation with better time resolution and obtain a
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