Our research is focussed on galactic and extragalactic
compact radio sources such as supernovae, pulsars, black hole candidates,
radio stars and the powerful cores of radio galaxies and quasars. With
the technique of very-long-baseline interferometry (VLBI) and a network
of several large radio telescopes girdling the globe, we are able to image
the areas of activity of these sources and determine their positions with
an angular resolution 1,000 times better than with any optical telescope
on Earth.
HOME