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combination of the CIGALE spectroscopic module with the 2D modules. They will then apply this new tool to the ALPINE CRISTAL sample to study the assembly of massive galaxies at z~5 using a very rich dataset
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archaeological and paleoseismological surveys to date sediments and/or rock surfaces by optically stimulated luminescence (OSL) affected by deformation (faults) or covered by collapsed megaliths. All of the data
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