%0 Journal Article %T Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process %A n_TOF Collaboration (Lederer, C. et al %A Giubrone, G. %A Domingo-Pardo, C. %A Tain, J. L. %J Nuclear Data Sheets %D 2014 %V 120 %I Academic Press Inc Elsevier Science %@ 0090-3752 %G English %F n_TOFCollaborationLederer_etal2014 %O WOS:000339860100056 %O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=1875), last updated on Sat, 30 Aug 2014 16:50:38 +0000 %X Neutron capture cross sections in the keV neutron energy region are the key nuclear physics input to study the astrophysical slow neutron capture process. In the past years, a series of neutron capture cross section measurements has been performed at the neutron time-of-flight facility n_TOF at CERN focussing on the Fe/Ni mass region. Recent results and future developments in the neutron time-of-flight technique are discussed. %R 10.1016/j.nds.2014.07.046 %U https://doi.org/10.1016/j.nds.2014.07.046 %P 201-204