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The neutron capture cross section of the s-process branch nucleus $^{63}$Niaffects the abundances of other nuclei in its region, especially $^{63}$Cu and$^{64}$Zn. In order to determine the energy dependent neutron capture crosssection in the astrophysical energy region, an experiment at the Los AlamosNational Laboratory has been performed using the calorimetric 4$\pi$ BaF$_2$array DANCE. The (n,$\gamma$) cross section of $^{63}$Ni has been determinedrelative to the well known $^{197}$Au standard with uncertainties below 15%.Various $^{63}$Ni resonances have been identified based on the Q-value.Furthermore, the s-process sensitivity of the new values was analyzed with thenew network calculation tool NETZ.

The $^{63}$Ni(n,$\gamma$) cross section measured with DANCE