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We present Karl G. Jansky Very Large Array radio frequency observations ofthe new accreting millisecond X-ray pulsar (AMXP), IGR J16597$-$3704, locatedin the globular cluster NGC 6256. With these data, we detect a radiocounterpart to IGR J16597$-$3704, and determine an improved source position.Pairing our radio observations with quasi-simultaneous Swift/XRT X-rayobservations, we place IGR J16597$-$3704 on the radio -- X-ray luminosityplane, where we find that IGR J16597$-$3704 is one of the more radio-quietneutron star low-mass X-ray binaries known to date. We discuss the mechanismsthat may govern radio luminosity (and in turn jet production and evolution) inAMXPs. Further, we use our derived radio position to search for a counterpartin archival Hubble Space Telescope and Chandra X-ray Observatory data, andestimate an upper limit on the X-ray luminosity of IGR J16597$-$3704 duringquiescence.

A radio frequency study of the accreting millisecond X-ray pulsar, IGR J16597$-$3704, in the globular cluster NGC 6256