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High Dynamical Range Observations on the VLT

Published online by Cambridge University Press:  26 May 2016

Anne M. Lagrange
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex
Gael Chauvin
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA
David Mouillet
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA
Jean-Luc Beuzit
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA
the NAOS Consortium
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA
the NAOS Consortium
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA
the NAOS Consortium
Affiliation:
Laboratoire d'Astrophysique de Grenoble; Université J. Fourier, BP 53; F38041 Grenoble Cedex ONERA

Abstract

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The recently installed Adaptive Optics system NAOS now offers diffraction limited images at the VLT. Together with the CONICA camera, NAOS provides the possibility to perform high dynamical range observations in the near IR domain. We present here NAOS-CONICA (hereafter NACO) capabilities as well as the first images of binaries obtained during NACO commissioning.

Type
Part 9. Future Prospects
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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