The main activities at the TIGO VLBI station during 2012 have been 120 successful VLBI sessions and the investigation of an alternate site for TIGO for future operation
In the framework of this thesis, the goal is to examine the planned VGOS network, which is currently...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
In 1984 an INTELSAT antenna of 32 m of diameter was constructed at 3 370 metres above the sea level ...
This report describes the status of the Matera VLBI station. Also, in an overview of the station, so...
The Wettzell RFI-Monitoring system was developed to monitor radio frequency interference at existing...
This is a brief report about the activities carried out at the Fortaleza geodetic VLBI station (ROEN...
General information about the Medicina Radio Astronomy Station, the 32-m antenna status, and the sta...
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory, which consists of...
In 2012, the German Antarctic Receiving Station (GARS) O'Higgins contributed to the IVS observing pr...
In the year 2012, the 20-m radio telescope at the Geodetic Observatory Wettzell, Germany again contr...
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory composed of a netw...
The Large Latin American Millimeter Array (LLAMA) is amultipurpose single-dish 12 m radiotelescope w...
During January and February 1990, 1991 and 1992 an important collaboration took place between the Ri...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
Current VLBI observations are controlled and attended locally at the radio telescopes on the basis o...
In the framework of this thesis, the goal is to examine the planned VGOS network, which is currently...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
In 1984 an INTELSAT antenna of 32 m of diameter was constructed at 3 370 metres above the sea level ...
This report describes the status of the Matera VLBI station. Also, in an overview of the station, so...
The Wettzell RFI-Monitoring system was developed to monitor radio frequency interference at existing...
This is a brief report about the activities carried out at the Fortaleza geodetic VLBI station (ROEN...
General information about the Medicina Radio Astronomy Station, the 32-m antenna status, and the sta...
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory, which consists of...
In 2012, the German Antarctic Receiving Station (GARS) O'Higgins contributed to the IVS observing pr...
In the year 2012, the 20-m radio telescope at the Geodetic Observatory Wettzell, Germany again contr...
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory composed of a netw...
The Large Latin American Millimeter Array (LLAMA) is amultipurpose single-dish 12 m radiotelescope w...
During January and February 1990, 1991 and 1992 an important collaboration took place between the Ri...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
Current VLBI observations are controlled and attended locally at the radio telescopes on the basis o...
In the framework of this thesis, the goal is to examine the planned VGOS network, which is currently...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
In 1984 an INTELSAT antenna of 32 m of diameter was constructed at 3 370 metres above the sea level ...