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O que (quem) é VLT Survey Telescope - definição
VLT Survey Telescope
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![CCD detectors]] that together create 268-megapixel images.](https://commons.wikimedia.org/wiki/Special:FilePath/OmegaCAM detectors VST eso1119j.jpg?width=200 "CCD detectors]] that together create 268-megapixel images.")
![VST's view of the [[Leo Triplet]] and beyond.](https://commons.wikimedia.org/wiki/Special:FilePath/VST's view of the Leo Triplet and beyond.jpg?width=200 "VST's view of the [[Leo Triplet]] and beyond.")
![Globular star cluster [[Omega Centauri]] as seen by the VST.](https://commons.wikimedia.org/wiki/Special:FilePath/VST image of the giant globular star cluster Omega Centauri.jpg?width=200 "Globular star cluster [[Omega Centauri]] as seen by the VST.")
WIDE-FIELD TELESCOPE ON CERRO PARANAL, CHILE
The VLT Survey Telescope (VST) is a telescope located at ESO’s Paranal Observatory in the Atacama Desert of northern Chile. It is housed in an enclosure immediately adjacent to the four Very Large Telescope (VLT) Unit Telescopes on the summit of Cerro Paranal.
NEOSTEL
AN ASTRONOMICAL SURVEY AND EARLY-WARNING SYSTEM FOR DETECTING NEAR-EARTH OBJECTS SIZED 40 M AND ABOVE A FEW WEEKS BEFORE THEY IMPACT EARTH
Near Earth Object Survey TELescope; Near Earth Object Survey Telescope; Flyeye Telescope; NEO Survey Telescope
The Near Earth Object Survey TELescope (NEOSTEL - also known as "Flyeye") is an astronomical survey and early-warning system for detecting near-Earth objects sized and above a few weeks before they impact Earth.
VIMOS-VLT Deep Survey
REDSHIFT SURVEY
VVDS; VIMOS-VLT Deep Survey (VVDS)
The VIMOS-VLT Deep Survey (VVDS) is a redshift survey carried out by a collaboration between French and Italian astronomical institutes using the VIMOS spectrograph, mounted on the telescope Melipal (UT3) of the Very Large Telescope, located at the Paranal Observatory in Chile.
