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MIDI, the 10 μm interferometer of the VLT

Published online by Cambridge University Press:  31 January 2003

G. Perrin ,
F. Malbet ,
G. Perrin ,
C. Leinert ,
U. Graser ,
L. B.F.M. Waters  and
B. Lopez
G. Perrin*
Affiliation:
LESIA, FRE 2461, Observatoire de Paris, Section de Meudon, 5 place Jules Janssen, 92190 Meudon, France;
C. Leinert
Affiliation:
Max-Planck-Institut für Astronomie, Koenigstuhl 17, 69117 Heidelberg, Germany;
U. Graser
Affiliation:
Max-Planck-Institut für Astronomie, Koenigstuhl 17, 69117 Heidelberg, Germany;
L. B.F.M. Waters
Affiliation:
Astronomical Institute, University of Amsterdam, Kruisland 403, 1098 SJ Amsterdam, The Netherlands;
B. Lopez
Affiliation:
Observatoire de la Côte d'Azur, BP. 4229, 06304 Nice, France;
*
guy.perrin@obspm.frleinert@mpia-hd.mpg.degraser@mpia-hd.mpg.derensw@astro.uva.nllopez@obs-nice.fr
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Abstract

We report in this paper on the current status of the mid-infrared beam combiner of the VLTI: MIDI. We explain the interest of VLTI for this range of wavelentghs and give an overview of the main characteristics of MIDI and present its scientific targets.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 6: Observing with the VLTI , 2003 , pp. 127
Copyright
© EAS, EDP Sciences, 2003

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