VST/OmegaCAM instrument specific query form now available
Published: 22 Dec 2011
The VLT Survey Telescope (VST) is a 2.6-m wide field optical survey telescope for the southern hemisphere located on the VLT platform at Cerro Paranal, Chile. It is equipped with just one focal plane instrument, OmegaCAM, a large format (16k x16k pixels) CCD camera built by an international consortium. It operates in the u,g,r,i,z SDSS bands, covering a corrected field of view of 1°x 1°.
The instrument specific VST/OmegaCAM query form is now available, remaining possible to access OmegaCAM data also via the main archive query form.
Access the VST/OmegaCAM specific query form here.