  An experimental method to determine the (n,g) cross section of short-living
s-process branching points using data of the inverse (g,n) reaction is
presented. The method was used to observe the branching point nucleus 95Zr
because the elemental abundance patterns corresponding to this branching point
cannot be reproduced by full stellar models and a possible error source is the
neutron capture cross section of 95Zr. The analysis of the experiment is still
under progress, we will outline the current status in this manuscript.
