EAS Publications Series
Volume 28, 2008Perspectives in Radiative Transfer and Interferometry
|Page(s)||1 - 8|
|Published online||22 April 2008|
S. Wolf, F. Allard and Ph. Stee (eds)
EAS Publications Series, 28 (2008) 1-8
The Very Large Telescope Interferometer
European Southern Observatory, Casilla 19001, Santiago, Chile
The Very Large Telescope Interferometer on Cerro Paranal in Northern Chile is one of the largest optical facilities used in astronomy. It can combine two or three of the four 8.2 m and four movable 1.8 m telescopes, which span baselines between 8 and 202 m. Observations are carried out in the near- and mid-infrared, covering the wavelength range from 1 to 13 μm.
© EAS, EDP Sciences, 2008
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