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The total cross sections for the $^{152}$Gd(p,$\gamma$)$^{153}$Tb and$^{152}$Gd(p,n)$^{152}$Tb reactions have been measured by the activation methodat effective center-of-mass energies \mbox{$3.47 \leqE_\mathrm{c.m.}^\mathrm{eff}\leq 7.94$ MeV} and \mbox{$4.96 \leqE_\mathrm{c.m.}^\mathrm{eff} \leq 7.94$ MeV}, respectively. The targets wereprepared by evaporation of 30.6\% isotopically enriched $^{152}$Gd oxide onaluminum backing foils, and bombarded with proton beams provided by a cyclotronaccelerator. The cross sections were deduced from the observed $\gamma$-rayactivity, which was detected off-line by a HPGe detector in a low backgroundenvironment. The results are presented and compared with predictions ofstatistical model calculations. This comparison supports a modified opticalproton+$^{152}$Gd potential suggested earlier.

Measurements of $^{152}$Gd(p,$\gamma$)$^{153}$Tb and $^{152}$Gd(p,n)$^{152}$Tb reaction cross sections for the astrophysical $\gamma$ process