- Startpagina tijdschrift
- Volume 74 - Année 2005
- Numéro 5 - 6
- Perspective of interometry in Antarctica
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Perspective of interometry in Antarctica
Proceedings of the European Interferometry Initiative Workshop organized in the context of the 20005 Joint European and National Astronomy Meeting "Distant Worlds"?
![Open Access](images/Open_Access.png)
Abstract
The recent Dome C site testing shows its potential for interferometry. This article presents a part of discussion about the site characteristics measured by E. Aristidi et al. during the polar night. In section 2, the site characteristics are described. In section 3, the Mykerinos prototype interferometer is exposed. This instrument can be the first step before the implementation of future large Antarctic interferometers. It will allow characterizing the best instrument specifications, test technology in extreme conditions, and check the performances predicted for interferometer from Dome C. Its baseline and precision will allow studies of hot Jupiters with small apertures.
Om dit artikel te citeren:
Over : B. Valat
Laboratoire Universitaire d’Astrophysique de Nice (LUAN) UMR 6525, France
Over : B. Lopez
Observatoire de la Côte d’Azur, Laboratoire Gemini UMR 6203, France
Over : F.X. Schmider
Laboratoire Universitaire d’Astrophysique de Nice (LUAN) UMR 6525, France
Over : F. Vakili
Laboratoire Universitaire d’Astrophysique de Nice (LUAN) UMR 6525, France
Over : E. Aristidi
Laboratoire Universitaire d’Astrophysique de Nice (LUAN) UMR 6525, France