Multi-aperture interferometry at Concordia

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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Bibliographische Detailangaben
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
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Atmosphere
Contributed Papers
Observatories
Radio astronomy
Radio telescopes
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Beschreibung
Zusammenfassung: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921307012343