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As an alternative production scenario to the so-called γ process, the most abundant p nucleus 92Mo may be produced by a chain of proton-capture reactions in supernovae type Ia. The reactions 90Zr(p,γ) and 91Nb(p,γ) are the most important reactions in this chain. We have measured the first reaction using high-resolution in-beam γ-spectroscopy at HORUS, Cologne, Germany, to contribute to the existing experimental data base. So far, we only investigated the high-energy part of the Gamow window and the analysis is still in progress. We plan to study the second reaction in standard kinematics at the FRANZ facility, Frankfurt, Germany. Current developments at FRANZ will be explained in detail.

Proton-capture reactions in thermonuclear supernovae and the p-process