Within the first year we finished the setup of the customised Laser Spectroscopy system, which included the automated sampling as well as the instant spectral analysis to gain climatic data.
We applied the method to mollusc shells from around the world and published elemental maps of oysters, clams and gastropods in the Journal of Analytical Atomic Spectroscopy (Hausmann et al. 2017).
The customised systems was then applied to a well established proxy for sea surface temperature in the Red Sea, Conomurex fasciatus.
However, the mollusc failed to produce sufficiently reliable elemental data for climate reconstruction. A comparison of the stable oxygen isotope values, which reflect sea surface temperature, and the Mg/Ca and Sr/Ca ratios has been accepted for publication by Springer, in the edited volume: Geological Setting of the Red Sea, by Najeeb Rasul and Ian Stewart.
The second year aimed to find other mollusc species to carry out climate reconstructions. By expanding our collaborative network to the US, Ireland, Australia, and Taiwan, we gained access to promising mollusc species, which yield high-resolution climatic data.
The most promising results were found in limpets and oysters.
The results of these collaborations are currently being written up and we aim to publish them in high impact journals (i.e. Nature Geoscience, PNAS).