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FLOATSUPERSCRIPT, surveying 61 potential sub-mJy and mJy radio source targets at angular resolution ranging from about 10 to 100 mas. Often a significant fraction of the total radio emission resides within a compact and unresolved radio "core", with a size measured on milliarcsecond (mas) and sub-mas scales using the techniques of very long baseline interferometry (VLBI). A total of 630 ksec of Chandra observing time was committed to this survey. Unlike traditional snapshot VLBI surveys, the wide-field approach permits many potential targets in the field to be imaged simultaneously, taking full advantage of the sensitivity and the coverage in the (u,v) plane associated with the total duration of the observations and the characteristics of the array. FLOATSUPERSCRIPT, detected a further 6 radio sources, drawn from 37 additional targets. POSTSUBSCRIPT%. This observational trend is expected from a rapidly evolving radio source population. 10. However, at these faint sensitivity levels it is increasingly difficult to identify radio-loud active galaxies from the dominant star forming radio source population, especially in the case of optically faint systems