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KMOS is one of the second generation instruments at the ESO-VLT and has been operating for five years. It has given us new insights into a variety of scientific topics such as galaxy formation and evolution, early stellar evolution and stellar populations. The KMOS@5 workshop will bring together scientists working on all areas of star and galaxy formation using near-infrared IFU spectroscopy, including results from complementary instruments. The five years milestone of KMOS offers a perfect opportunity to assess the impact of this instrument on its core science cases and to look forward to develop new strategies and programs, also in light of future IFU instruments.