Abstract
Improving the performances of basic optical functions (splitting, directional coupling, phase modulation) is compulsory for the development of new astronomical instruments based on integrated optics. In particular, for the mid-infrared domain, where a number of projects are being developed (ASGAARD-NOTT instrument for VLTI [1], METIS for EELT [2] or future spatial projects such as LIFE [3]), these functions have to be validated in terms of achromaticy, polarization dependence and transmission losses.
© 2023 IEEE
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