Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ti</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>44</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction relevant for supernova nucleosynthesis
Christof Vockenhuber(ETH Zurich), A. Wallner(Australian National University), C.O. Ouellet, Evan O’Connor, R. Lewis, H. L. Crawford(Lawrence Berkeley National Laboratory), L. M. R. Fogarty(The University of Sydney), D. Frekers(University of Münster), G. Ruprecht, D. Ottewell, A. A. Chen, B. Davids, W. Kutschera(University of Vienna), Camilo Ruíz(University of Bern), M. Trinczek, M. Paul(Hebrew University of Jerusalem), A. Hussein, Lih‐Sin The, J. Pearson, B. Wales, L. Buchmann, M. M. Pavan, J.M. D’Auria, A. M. Laird, J. A. Caggiano(Lawrence Livermore National Laboratory), D.A. Hutcheon
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