Precise measurement of the thermal and stellar <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">Fe</mml:mi><mml:mprescripts/><mml:none/><mml:mn>54</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Fe</mml:mi><mml:mprescripts/><mml:none/><mml:mn>55</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> cross sections via accelerator mass spectrometry
A. Wallner(Australian National University), László Szentmiklósi(HUN-REN Centre for Energy Research), R. Reifarth(Goethe University Frankfurt), M. Pignatari(Konkoly Observatory), I. Dillmann(GSI Helmholtz Centre for Heavy Ion Research), K. Buczak(University of Vienna), Peter Steier(University of Vienna), T. Belgya(HUN-REN Centre for Energy Research), Robin Golser(University of Vienna), W. Kutschera(University of Vienna), L. Coquard(Karlsruhe Institute of Technology), Amanda I. Karakas(ASTRO-3D), M. Bichler(Schott (Germany)), A. Mengoni(International Atomic Energy Agency), C. Lederer(University of Vienna), F. Käppeler(FZI Research Center for Information Technology), Alfred Priller(University of Vienna)
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