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will include an important component of code development, in order to produce multi-color light curves of supernovae in 1D simulations that account for the physics of the stellar core (nucleosynthesis and
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-free analysis and/or relaxation dispersion measurements and their interpretation In-cell NMR or NMR of bacterial suspensions or similar hrMAS NMR and/or solid-state NMR of membrane-bound peptides
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