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We hope to transform an instrument like the first-focus one of the LBT into the spearhead facility to identify the multiple populations in galactic globular clusters from the ground.
A new set of simulations has been developed to identify the best thin-layer filter to be used in order to separate populations with different light element abundances. We also built an optomechanical set-up to test the filter behavior in a LBC-like configuration. We present here the simulation strategy and some transmission curve obtained with the laboratory set-up.
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