European VLBI Network observations of fourteen GHz-Peaked-Spectrum radio   sources at 5 GHz
  We present the results of EVN polarization observations of fourteen GHz-Peaked-Spectrum (GPS) radio sources at 5 GHz. These sources were selected from bright GPS source samples and we aimed at finding Compact Symmetric Objects (CSOs). We have obtained full polarization 5 GHz VLBI observations of 14 sources providing information on their source structure and spectral indices. The results show that two core-jet sources 1433$-$040 and DA193, out of 14 GPS sources, exhibit integrated fractional polarizations of 3.6% and 1.0% respectively. The other 12 sources have no clear detection of pc-scale polarization. The results confirm that the GPS sources generally have very low polarization at 5 GHz. The sources 1133+432, 1824+271 and 2121$-$014 are confirmed as CSOs. Three new CSOs 0914+114, 1518+046 and 2322$-$040 (tentative) have been classified on the basis of 5 GHz images and spectral indices. The sources 1333+589, 1751+278 and 2323+790 can be classified either as compact doubles, and then they are likely CSO candidates or core-jet sources; further observations are needed for an appropriate classification; 0554$-$026, 1433$-$040 and 1509+054 are core-jet sources. In addition, we estimate that a component in the jet of quasar DA193 has superluminal motion of $3.3\pm0.6 h^{-1}c$ in 5.5 years. 
Liu Xiang (Urumqi Observatory, NAOC), Cormac Reynolds (JIVE), Richard   Strom (ASTRON) and Daniele Dallacasa (INAF)