Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T05:51:05.305Z Has data issue: false hasContentIssue false

A STEP: Towards a Large Photometric Survey for Exoplanets at Dome C

Published online by Cambridge University Press:  23 May 2007

F. Fressin
Affiliation:
Observatoire de la Côte d'Azur
T. Guillot
Affiliation:
Laboratoire Universitaire Astrophysique de Nice
F.-X. Schmider
Affiliation:
Laboratoire Universitaire Astrophysique de Nice
A. Agabi
Affiliation:
Laboratoire d'Astrophysique de Marseille
C. Moutou
Affiliation:
Laboratoire d'Astrophysique de Marseille
S. Aigrain
Affiliation:
University of Exeter
F. Bouchy
Affiliation:
Observatoire de Haute Provence
M. Boer
Affiliation:
Observatoire de Haute Provence
F. Pont
Affiliation:
Observatoire de Genêve
A. Erikson
Affiliation:
Berlin DLR
H. Rauer
Affiliation:
Berlin DLR
Get access

Abstract

We present “A STEP” (Antarctica Search for Transiting ExtrasolarPlanets), a project dedicated to the search for planetary transitsfrom Antartica. The project consists of a semi-automatic ~40 cmtelescope equipped with a 16-million-pixel CCD installed at DomeC. The site offers crucial assets for a ground-based exoplanet transitsearch: uninterrupted phase coverage, excellent weather, low air-massvariations and reduced scintillation.
This system would be able to detect Pegasids transiting in front ofstars as faint as magnitude sixteen and could also detect smallerplanets in close-in period around brighter stars. This short termproject is meant to be a photometric qualifyer for the site and thefirst stage of a massive detection campaign. A mid-term objective of1000 detections for 2012 could be achieved either with many smalltelescopes or with a large Schmidt telescope with a large field ofview.
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 and cold temperaturequalification.


Type
Research Article
Copyright
© EAS, EDP Sciences, 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)