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Multi-aperture interferometry at Concordia

Published online by Cambridge University Press:  01 August 2006

Eric Fossat ,
Farrokh Vakili ,
Eric Aristidi ,
Bruno Lopez ,
François-Xavier Schmider ,
Karim Agabi ,
Jean-Baptiste Daban ,
Fatmé Allouche ,
Adrian Belu  and
Pierre-Marie Gori
...Show all authors
Eric Fossat
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Farrokh Vakili
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Eric Aristidi
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Bruno Lopez
Affiliation:
Observatoire de la cote d'Azur, BP 4229, F-06304 Nice, France
François-Xavier Schmider
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Karim Agabi
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Jean-Baptiste Daban
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Fatmé Allouche
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Adrian Belu
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Pierre-Marie Gori
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Géraldine Guerri
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
Bruno Valat
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: [email protected]
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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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 705 - 706
Copyright
Copyright © International Astronomical Union 2007

References

Labeyrie, A., Le Coroller, H., Dejonghe, J., et al. 2003, SPIE, 4852, 236Google Scholar
Vakili, F., Aristidi, E., Abe, L., & Lopez, B. 2004, A&A, 421, 147Google Scholar