  Five compact radio sources, include 0420-014, 1334-127, 1504-166, 2243-123,
and 2345-167, were observed at 5GHz by European VLBI (Very Long Baseline
Interferometry) Network (EVN) in June, 1996. The primary purpose of this
observation was to confirm their superluminal proper motions. Here, the results
of 1334-127, 1504-166, 2243-123 and 2345-167 are presented.
