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Archival ALMA continuum data was also utilized.\n  Results: At least 40 jet knots were identified via NIR emission from H$_2$ and [FeII] tracing shocked gas. Bright jet knots outflowing from the central most massive protostar, S4, are detected towards the east of the source and are resolved in fine detail with the AO imaging. Additional knots are distributed throughout the","authors_text":"A. Caratti o Garatti, A. Gautam, A. Puglisi, B. Rothberg, C. Plantet, C. Veillet, D. Miller, E. Ghose, E. Pinna, F. Rossi, G. Agapito, G. Brusa, G. Cosentino, G. Taylor, J. Christou, J. C. Tan, J.P. Farias, J. Power, K. Tanaka, M. Andersen, M. Bonaglia, M. Grudic, M. Whittle, R. Briguglio, R. Fedriani, R. Garcia-Lopez, S. Crowe, S. Esposito, T. Mazzoni, V. Rosero, X. Zhang, Y. Zhang, Z. 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