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Accurate modeling of astrophysical jets is critical for understandingaccretion systems and their impact on the interstellar medium. Whileastronomical observations can validate models, they have limitations.Controlled laboratory experiments offer a complementary approach forqualitative and quantitative demonstration. Laser experiments offer acomplementary approach. This article introduces a new platform on the OMEGAlaser facility for high-velocity (1500 km/s), high-aspect-ratio ($\sim$36) jetcreation with strong cylindrical symmetry. This platform s capabilities bridgeobservational gaps, enabling controlled initial conditions and directmeasurements

Development of a platform for experimental and computational studies of magnetic and radiative effects on astrophysically-relevant jets at OMEGA