The VLT Survey Telescope (VST) is a 2.6m aperture, wide field, UV to I facility, to be installed at the European Southern Observatory (ESO) on the Cerro Paranal Chile. VST was primarily intended to complement the observing capabilities of VLT with wide-angle imaging for detecting and pre-characterising sources for further observations with the VLT.
@article{arxiv.astro-ph/0501598,
title = {VST - VLT Survey Telescope Integration Status},
author = {C. Belfiore and M. Brescia and M. Capaccioli and O. Caputi and G. Castiello and F. Cortecchia and L. Ferragina and D. Fierro and V. Fiume and D. Mancini and G. Mancini and G. Marra and L. Marty and G. Mazzola and L. Parisi and L. Pellone and F. Perrotta and V. Porzio and P. Schipani and G. Sciarretta and G. Spirito and M. Valentino and G. Sedmak},
journal= {arXiv preprint arXiv:astro-ph/0501598},
year = {2007}
}