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Antarctica Search for Transiting Extrasolar Planets

Published online by Cambridge University Press:  05 January 2006

F. Fressin
Affiliation:
Observatoire de la Côte d'Azur, France
T. Guillot
Affiliation:
Observatoire de la Côte d'Azur, France
F. Bouchy
Affiliation:
Laboratoire d'Astrophysique de Marseille, France
A. Erikson
Affiliation:
Berlin DLR
J. Gay
Affiliation:
Observatoire de la Côte d'Azur, France
A. Léger
Affiliation:
Institut d'Astrophysique Spatiale
F. Pont
Affiliation:
Observatoire de Genêve
H. Rauer
Affiliation:
Berlin DLR
J.-P. Rivet
Affiliation:
Observatoire de la Côte d'Azur, France
F. Valbousquet
Affiliation:
Optique et Vision
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Abstract

We present “A STEP”, a project dedicated to the search for planetarytransits from Antartica. The project consists of a fully automatic 40 cm telescope equipped with an 11-million-pixel CCD installed atDome C. The site offers crucial assets for a ground-based exoplanettransit search: uninterrupted phase coverage and excellentseeing. 
This system would be able to detect hot Jupiters transiting in frontof stars as faint as magnitude sixteen and could also detect smallerplanets in close-in period around brighter stars. Our estimations,based on results of previous surveys are an average of 6 detectionsper 60 days survey. Compared to existing surveys, this excellent yieldis due to the nearly-continuous phase coverage and excellent seiing.This short term project is meant to be a photometric qualifyer for thesite and the first stage of a massive detection campaign. A mid-termobjective of 1000 detections for 2012 could be achieved either with manysmall telescopes or with a large Schmidt telescope with a large fieldof view. 
The project is relatively simple and cost-effective, and has thedouble purpose of qualifying the site and obtaining first-classscientific results. Our team is already familiar with transitdetection with an automated telescope (BEST) and cold temperaturequalification.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2005

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