EAS Publications Series
Volume 40, 20103rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)
|Page(s)||257 - 262|
|Published online||23 December 2009|
L. Spinoglio and N. Epchtein (eds)
EAS Publications Series, 40 (2010) 257-262
Exozodiacal discs with ALADDIN: how faint can we detect them?
Department of Astrophysics, Geophysics and Oceanography, University of Liège, Belgium
2 LESIA, Observatoire de Paris-Meudon, France
3 Thalès-Alenia Space, Cannes-La Bocca, France
4 Netherlands Institute for Space Research (SRON), Utrecht, The Netherlands
In this paper, we describe the expected performance of ALADDIN, a nulling interferometer project optimised for operation at Dome C. After reviewing the main atmospheric parameters pertaining to infrared interferometry on the high Antarctic plateau, we shortly describe the ALADDIN instrument and compute its estimated performance in terms of the smallest exozodiacal dust disc density that can be detected. Our estimations are based on a thorough end-to-end software simulator previously developed for the GENIE nulling interferometer project at VLTI. We then propose a possible mission scenario, where the southern target stars of future exo-Earth characterisation missions can be surveyed for the presence of bright exozodiacal discs (>50 zodi) within one winter-over at Concordia.
© EAS, EDP Sciences, 2010
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