Abstract
Twenty-five small-diameter radio sources have been observed at 15.4 GHz with the Cambridge 5-km telescope. A method which uses an unresolved component in the field of view as a phase reference has been developed in order to search for faint outer structure around bright compact objects. Maps are presented for 11 of the sources. It is suggested that all sources selected in low-frequency surveys have outer structure on scales > 0.5 arcsec.

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