Add to ORKGAbstract. The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approaching completion. After the four 8-m Unit Telescopes (UT) individually saw first light in the last years, two of them were combined for the first time on October 30, 2001 to form a stellar interferometer, the VLT Inter-ferometer. The combination in pairs of all four UTs was completed in September 2002. In this article, we will describe the subsystems of the VLTI and the planning for the following years
ESO is building the Phase Referenced Imaging and Microarcsecond Astronomy (PRIMA) facility for the V...
Recent advances in the development of interferometric instruments coupled to long baseline facilitie...
The VST (Very Large Telescope Survey Telescope) is an 2.6 m class Alt-Az telescope which will be ins...
The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approachin...
The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approac...
We present the latest update of the European Southern Observatory’s Very Large Telescope interferome...
In this article we present the Data Flow System (DFS) for the Very Large Telescope Interferometer (V...
The Very Large Telescope Interferometer on Cerro Paranal in Northern Chile is one of the largest opt...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
Observatory and in Europe, progressed very well. On the following pages is a brief description of th...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
unanimously decided that the world's large3 opticat telescope, the 1 &metre equivalent very...
Optical interferometers are instruments that combine the light coming from separated optical telesc...
Installed at the heart of the Very Large Telescope Interferometer (VLTI), VINCI combines coherently ...
The last decade has seen VLTI transitioning from 2 to 3 to 4 Telescopes recombination. This led to a...
ESO is building the Phase Referenced Imaging and Microarcsecond Astronomy (PRIMA) facility for the V...
Recent advances in the development of interferometric instruments coupled to long baseline facilitie...
The VST (Very Large Telescope Survey Telescope) is an 2.6 m class Alt-Az telescope which will be ins...
The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approachin...
The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approac...
We present the latest update of the European Southern Observatory’s Very Large Telescope interferome...
In this article we present the Data Flow System (DFS) for the Very Large Telescope Interferometer (V...
The Very Large Telescope Interferometer on Cerro Paranal in Northern Chile is one of the largest opt...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
Observatory and in Europe, progressed very well. On the following pages is a brief description of th...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
unanimously decided that the world's large3 opticat telescope, the 1 &metre equivalent very...
Optical interferometers are instruments that combine the light coming from separated optical telesc...
Installed at the heart of the Very Large Telescope Interferometer (VLTI), VINCI combines coherently ...
The last decade has seen VLTI transitioning from 2 to 3 to 4 Telescopes recombination. This led to a...
ESO is building the Phase Referenced Imaging and Microarcsecond Astronomy (PRIMA) facility for the V...
Recent advances in the development of interferometric instruments coupled to long baseline facilitie...
The VST (Very Large Telescope Survey Telescope) is an 2.6 m class Alt-Az telescope which will be ins...