Multi-aperture interferometry at Concordia

The next generation (post-VLTI) of multi-telescope interferometric arrays operated in optical/infrared wavelengths should be kilometric, from 1 to 10 km. The Concordia station offers a unique opportunity to set such an interferometer in the best atmospheric conditions presently known on Earth.

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Veröffentlicht in:Proceedings of the International Astronomical Union 2006-08, Vol.2 (14), p.705-706
Hauptverfasser: Fossat, Eric, Vakili, Farrokh, Aristidi, Eric, Lopez, Bruno, Schmider, François-Xavier, Agabi, Karim, Daban, Jean-Baptiste, Allouche, Fatmé, Belu, Adrian, Gori, Pierre-Marie, Guerri, Géraldine, Valat, Bruno
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Sprache:eng
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