Abstract
The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approaching completion this year, when the fourth of the 8-m Unit Telescopes will see first light. At the same time, the preparation for first fringes of the VLT Interferometer (VLTI) is advancing rapidly with the goal of having the first fringes with two siderostats in the first quarter of 2001. In this article we describe the status of the VLTI and its subsystems, we discuss the planning for first fringes with the different telescopes and instruments. In conclusion, we present an outlook for the future of interferometry with Very Large Telescopes.
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More From: Comptes Rendus de l'Academie des Sciences Series IV Physics
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