OmegaCAM at the VLT Survey Telescope

  • E. Cappellaro
  • , A. Baruffolo
  • , E. Cascone
  • , L. Greggio
  • , K. Kuijken
  • , R. Bender
  • , B. Muschielok
  • , O. Iwert
  • , W. Mitsch
  • , H. Nicklas
  • , E. A. Valentijn

Research output: Contribution to journalArticleAcademicpeer-review

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 languageEnglish
Pages (from-to)967
JournalMemorie della Societa Astronomica Italiana
Volume74
Publication statusPublished - 2003

Keywords

  • Instrumentation: detectors
  • Surveys

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