摘要: The Seoul Radio Astronomy Observatory (SRAO) operates a 6.1-meter radio
telescope on the Gwanak campus of Seoul National University. We present the
efforts to reform SRAO to a Very Long Baseline Interferometry (VLBI) station,
motivated by recent achievements by millimeter interferometer networks such as
Event Horizon Telescope, East Asia VLBI Network, and Korean VLBI Network (KVN).
For this goal, we installed a receiver that had been used in the Combined Array
for Research in Millimeter-wave Astronomy and a digital backend, including an
H-maser clock. The existing hardware and software were also revised, which had
been dedicated only to single-dish operations. After several years of
preparations and test observations in 1 and 3-millimeter bands, a fringe was
successfully detected toward 3C 84 in 86 GHz in June 2022 for a baseline
between SRAO and KVN Ulsan station separated by 300 km. Thanks to the dual
frequency operation of the receiver, the VLBI observations will soon be
extended to the 1 mm band and verify the frequency phase referencing technique
between 1 and 3-millimeter bands.