We invite proposals for the open use observations of the KaVA. It will provide opportunities of VLBIobservations at 22 and 43 GHa for astronomers in the world.The very long baseline interferornetry (VLBI) technique offers angular resolutions superior to any other irsstruments at other wavelengths,enabling unique science applications of high-resolution imaging of radio sources and high-precision astrometry.The East Asia VLBI Network(EAVN) is a collabarative effort in the fast Asian region.
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