  The reaction network in the neutron-deficient part of the nuclear chart
around $A \sim 100$ contains several nuclei of importance to astrophysical
processes, such as the p-process. This work reports on the results from recent
experimental studies of the radiative proton-capture reactions
$^{112,114}\mathrm{Cd}(p,\gamma)^{113,115}\mathrm{In}$. Experimental cross
sections for the reactions have been measured for proton beam energies residing
inside the respective Gamow windows for each reaction, using isotopically
enriched $^{112}\mathrm{Cd}$ and $^{114}\mathrm{Cd}$ targets. Two different
techniques, the in-beam $\gamma$-ray spectroscopy and the activation method
have been employed, with the latter considered necessary to account for the
presence of low-lying isomers in $^{113}\mathrm{In}$ ($E_{\gamma} \approx
392$~keV, $t_{1/2} \approx 100$~min), and $^{115}\mathrm{In}$ ($E_{\gamma}
\approx 336$~keV, $t_{1/2} \approx 4.5$~h). Following the measurement of the
total reaction cross sections, the astrophysical S factors have been
additionally deduced. The experimental results are compared with
Hauser-Feshbach theoretical calculations carried out with the most recent
version of TALYS. The results are discussed in terms of their significance to
the various parameters entering the models.
