VLBI imaging of extremely high redshift quasars at 5 GHz

Details VLBI imaging of extremely high redshift quasars at 5 GHz VLBI imaging of extremely high redshift quasars at 5 GHz

1999-01-28

arxiv.org/abs/astro-ph/9901396v1

Astron.Astrophys.344:51,1999

Astronomy and Astrophysics

Astrophysics

Astronomy and Astrophysics, in press, Latex2e, 10 pages, 3 figures (and lots of sub-figures)

Scientific paper

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 asymmetric structure. The sample includes 1428+423, the most distant radio loud quasar known to date (z=4.72). It is barely resolved with an angular resolution of about 2.0*1.4 mas.

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