We present very long baseline interferometry (VLBI) images of ten very high redshift ( z> 3) quasars at 5 GHz. The sources 0004+139, 0830+101, 0906+041, 0938+119 and 1500+045 were observed in September 1992 using a global VLBI array, while 0046+063, 0243+181, 1338+381, 1428+423 and 1557+032 were observed in October 1996 with the European VLBI Network and Hartebeesthoek, South Africa. Most of the sources are resolved and show asym- metric structure. The sample includes 1428+423, the most dis- tant radio loud quasar known to date (z =4 :72). It is barely resolved with an angular resolution of about 2.01.4 mas.

VLBI imaging of ten very high redshift quasars at 5 GHz reveals asymme- metric structures and resolves most sources, including 1428+423, the most distant radio loud quasar known to date.

VLBI imaging of extremely high redshift quasars at 5 GHz

Key Takeaway: VLBI imaging of ten very high redshift quasars at 5 GHz reveals asymme- metric structures and resolves most sources, including 1428+423, the most distant radio loud quasar known to date.