Add to ORKGThe Sejong VLBI station officially joined the IVS as a new Network Station in 2012. This report summarizes the activities of the Sejong station during 2012. The following are the activities at the station: 1) VLBI test observations were carried out with the Tsukuba 34-m antenna of the GSI in Japan. As a result, the Sejong antenna needs to improve its efficiency, which is currently in progress, 2) A survey to connect the VLBI reference point to GNSS and ground marks was conducted, and 3) To see the indirect effects of RFI (Radio Frequency Interference) at this place, we checked the omni-direction (AZ 0 to 360, EL fixed at 7) for RFI influence
The New Zealand 12-m antenna is scheduled to start participating in regular IVS VLBI sessions from t...
The Kashima 34-m radio telescope has been continuously operated and maintained by the National Insti...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
A permanent geodetic VLBI station with a 22-m diameter antenna will be newly constructed in Korea by...
The Tsukuba 32-m VLBI station is operated by the Geospatial Information Authority of Japan. This rep...
Two 11-m VLBI antennas at Kashima and Koganei are continuously operated and maintained by the Nation...
This report summarizes the observing activities at the Sheshan station (SESHAN25) in 2012. It includ...
The K5/VSSP software correlator (Figure 1), located in Tsukuba, Japan, is operated by the Geospatial...
Korea's new VLBI project to construct the Korean VLBI Network (KVN) started in 2001, as a 7-year pro...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
The Japanese lunar explorer SELENE (SElenological and Engineering Explorer), to be launched in 2007,...
From October 2003 to September 2005, the International VLBI Service for Geodesy and Astrometry (IVS)...
This report summarizes information about the Svetloe Radio Astronomical Observatory activities in 20...
The first phase of the Korea-Japan Joint VLBI Correlator (KJJVC) development has been completed and ...
The Japanese lunar explorer SELENE (KAGUYA), which has been launched on Sep. 14th, 2007, utilizes VL...
The New Zealand 12-m antenna is scheduled to start participating in regular IVS VLBI sessions from t...
The Kashima 34-m radio telescope has been continuously operated and maintained by the National Insti...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
A permanent geodetic VLBI station with a 22-m diameter antenna will be newly constructed in Korea by...
The Tsukuba 32-m VLBI station is operated by the Geospatial Information Authority of Japan. This rep...
Two 11-m VLBI antennas at Kashima and Koganei are continuously operated and maintained by the Nation...
This report summarizes the observing activities at the Sheshan station (SESHAN25) in 2012. It includ...
The K5/VSSP software correlator (Figure 1), located in Tsukuba, Japan, is operated by the Geospatial...
Korea's new VLBI project to construct the Korean VLBI Network (KVN) started in 2001, as a 7-year pro...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
The Japanese lunar explorer SELENE (SElenological and Engineering Explorer), to be launched in 2007,...
From October 2003 to September 2005, the International VLBI Service for Geodesy and Astrometry (IVS)...
This report summarizes information about the Svetloe Radio Astronomical Observatory activities in 20...
The first phase of the Korea-Japan Joint VLBI Correlator (KJJVC) development has been completed and ...
The Japanese lunar explorer SELENE (KAGUYA), which has been launched on Sep. 14th, 2007, utilizes VL...
The New Zealand 12-m antenna is scheduled to start participating in regular IVS VLBI sessions from t...
The Kashima 34-m radio telescope has been continuously operated and maintained by the National Insti...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...