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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: eric.fossat@unice.fr
Farrokh Vakili
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Eric Aristidi
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
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: eric.fossat@unice.fr
Karim Agabi
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Jean-Baptiste Daban
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Fatmé Allouche
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Adrian Belu
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Pierre-Marie Gori
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Géraldine Guerri
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
Bruno Valat
Affiliation:
LUAN, UMR 6525, Université de Nice – Sophia Antipolis, Parc Valrose, F-06108 Nice, France email: eric.fossat@unice.fr
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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.

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