The most distant radio quasars at the highest resolution
  There are about 50 quasars known at redshifts z>5.7 to date. Only three of
them are detected in the radio (J0836+0054, z=5.77; J1427+3312, z=6.12;
J1429+5447, z=6.21). The highest-redshift quasars are in the forefront of
current astrophysical and cosmological research since they provide important
constraints on the growth of the earliest supermassive black holes in the
Universe, and on the physical conditions in their environment. These sources
are indeed associated with active galactic nuclei as revealed by
high-resolution Very Long Baseline Interferometry (VLBI) observations. It is
still unclear whether the physical properties of the few z~6 radio quasars are
in general similar to those of their lower-redshift cousins. In the case of
J1427+3312, the 100-pc scale double morphology suggests a young radio source.
Here we report on the recent European VLBI Network (EVN) imaging observations
of J1429+5447, the most distant radio quasar known. Based on its
milli-arcsecond-scale structural and spectral properties, this quasar is
similar to J0836+0054 and J1427+3312. This raises the question if the compact
steep-spectrum radio emission is a "universal" feature of the most distant
radio quasars. It could only be answered after many more objects at z>6 are
discovered and studied.
