EAS Publications Series
Volume 6, 2003Observing with the VLTI
|Page(s)||127 - 127|
|Published online||31 January 2003|
G. Perrin and F. Malbet (eds)
EAS Publications Series, 6 (2003) 127
MIDI, the 10 μm interferometer of the VLT
LESIA, FRE 2461, Observatoire de Paris,
Section de Meudon, 5 place Jules Janssen, 92190 Meudon, France;
2 Max-Planck-Institut für Astronomie, Koenigstuhl 17, 69117 Heidelberg, Germany;
3 Astronomical Institute, University of Amsterdam, Kruisland 403, 1098 SJ Amsterdam, The Netherlands;
4 Observatoire de la Côte d'Azur, BP. 4229, 06304 Nice, France;
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.
© EAS, EDP Sciences, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.