<sup>60</sup>Fe and<sup>244</sup>Pu deposited on Earth constrain the r-process yields of recent nearby supernovae
A. Wallner(Australian National University), Takeyasu Yamagata(The University of Tokyo), Maki Honda(University of Tsukuba), M.B. Froehlich(Australian National University), Norikazu Kinoshita(Kanazawa University), D. Schumann(Paul Scherrer Institute), M.A.C. Hotchkis(Australian Nuclear Science and Technology Organisation), Stefan Pavetich(Australian National University), Martin Martschini(Australian National University), M. Paul(Hebrew University of Jerusalem), Hideaki Matsuzaki(NTT (Japan)), N. Kivel(Paul Scherrer Institute), S.G. Tims(Australian National University)
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