Bildunterschrift
Figure 1: Comparision of a theoretical (DFT) Raman spectrum of a non-defective primitive In2O3 cell (red) and an in situ 385 nm Raman spectrum (blue) of In2O3 recorded at 25 °C in 25% O2/H2. The asterisks (*) mark bands originating from the CaF2 window, while the sharp feature at around 650 cm–1 results from cosmic rays.
