The first phase of the Korea-Japan Joint VLBI Correlator (KJJVC) development has been completed and installed to correlate the observed data from KVN (Korean VLBI Network) and VERA (VLBI Exploration of Radio Astrometry) in October 2009. KJJVC is able to process 16 stations, a maximum of 8 Gbps/station, and 8,192 output channels for VLBI data. The system configuration, the experimental results, and future plans are introduced in this paper
This report summarizes the activities of the Shanghai VLBI Correlator during 2012
The Sejong VLBI station officially joined the IVS as a new Network Station in 2012. This report summ...
In order to search for new VLBI sources in the Galactic plane that can be used as phase reference so...
Korea-Japan Joint VLBI Correlator (KJJVC) is being developed by collaborating KASI (Korea Astronomy ...
Korea's new VLBI project to construct the Korean VLBI Network (KVN) started in 2001, as a 7-year pro...
We report results of the performance evaluation of a new hardware correlator in Korea, the Daejeon c...
We present the basic features and the activities of Japanese VLBI network (JVN), a newly-established...
Korean VLBI Network (KVN) is the rst dedicated mm-wavelength VLBI Network in East Asia and will be a...
The K5/VSSP software correlator (Figure 1), located in Tsukuba, Japan, is operated by the Geospatial...
A permanent geodetic VLBI station with a 22-m diameter antenna will be newly constructed in Korea by...
VLBI technology development made significant progress at SHAO in the last few years. The development...
The East Asian VLBI Network (EAVN) is an international VLBI facility in East Asia and is operated un...
High-frequency very long baseline interferometry (VLBI) observations have made remarkable progress i...
The software correlator of the Chinese VLBI Network (CVN) has played an irreplaceable role in the CV...
The KVN(Korean VLBI Network)-style simultaneous multi-frequency receiving mode is demonstrated to be...
This report summarizes the activities of the Shanghai VLBI Correlator during 2012
The Sejong VLBI station officially joined the IVS as a new Network Station in 2012. This report summ...
In order to search for new VLBI sources in the Galactic plane that can be used as phase reference so...
Korea-Japan Joint VLBI Correlator (KJJVC) is being developed by collaborating KASI (Korea Astronomy ...
Korea's new VLBI project to construct the Korean VLBI Network (KVN) started in 2001, as a 7-year pro...
We report results of the performance evaluation of a new hardware correlator in Korea, the Daejeon c...
We present the basic features and the activities of Japanese VLBI network (JVN), a newly-established...
Korean VLBI Network (KVN) is the rst dedicated mm-wavelength VLBI Network in East Asia and will be a...
The K5/VSSP software correlator (Figure 1), located in Tsukuba, Japan, is operated by the Geospatial...
A permanent geodetic VLBI station with a 22-m diameter antenna will be newly constructed in Korea by...
VLBI technology development made significant progress at SHAO in the last few years. The development...
The East Asian VLBI Network (EAVN) is an international VLBI facility in East Asia and is operated un...
High-frequency very long baseline interferometry (VLBI) observations have made remarkable progress i...
The software correlator of the Chinese VLBI Network (CVN) has played an irreplaceable role in the CV...
The KVN(Korean VLBI Network)-style simultaneous multi-frequency receiving mode is demonstrated to be...
This report summarizes the activities of the Shanghai VLBI Correlator during 2012
The Sejong VLBI station officially joined the IVS as a new Network Station in 2012. This report summ...
In order to search for new VLBI sources in the Galactic plane that can be used as phase reference so...