Abstract
We present the status of the VLT Survey Telescope (VST) and OmegaCAM
projects. VST is a 2.6m telescope which will be integrated in the
ESO-VLT environment at Paranal and will be equipped with a 16k ×
16k CCD camera (OmegaCAM) covering 1 square degree with a resolution of
0.21 arcsec/pix. The main scope of this observing facility is the
selection of targets for VLT science. It is expected that VST+OmegaCAM
will become operational in spring 2004.
| Original language | English |
|---|---|
| Pages (from-to) | 967 |
| Journal | Memorie della Societa Astronomica Italiana |
| Volume | 74 |
| Publication status | Published - 2003 |
Keywords
- Instrumentation: detectors
- Surveys