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The capture cross section of $^{209}$Bi(n,$\gamma$)$^{210g}$Bi was measuredat different astrophysically energies including thermal capture cross section(25 meV), resonance integral, and the Maxwellian averaged cross section at athermal energy of $kT$ = 30 keV. The partial capture cross section ($\sigma_g$)was determined using the activation technique and by measuring the $^{210}$Poactivity. The newly developed and tested NICE detector setup was used tomeasure the $\alpha$-activity of the $^{210}$Po. Using this setup the thermaland resonance integral cross sections were determined to be$16.2\;\pm\;0.97$~mb and $89.81\;\pm\;8.0$~mb, respectively. And the Maxwellianaverage cross section was measured to be $2.01\;\pm\;0.38$~mb.

Determination of the $^{209}$Bi(n,$\gamma$)$^{210g}$Bi cross section using the NICE-Detector