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Science with ICE-T: Exoplanets and stellar/solar activity

Published online by Cambridge University Press:  13 November 2008

K.G. Strassmeier
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
T. Granzer
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
C. Denker
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
C. Fuhrmann
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
D. Fügner
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
M. Woche
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
I. DiVarano
Affiliation:
Astrophysical Institute Potsdam (AIP), Potsdam, Germany
G. Cutispoto
Affiliation:
INAF – Catania Astrophysical Observatory, Catania, Italy
A. Herber
Affiliation:
Alfred-Wegener-Institute for Polar and Marine Research (AWI), Bremerhaven, Germany
K. Horne
Affiliation:
University of St-.Andrews, Scotland, UK
P. Rafanelli
Affiliation:
Istituto Astronomico, Universtà degli Studi Padova, Padova, Italy
F. Bortoletto
Affiliation:
INAF–Osservatorio Astronomico di Padova, Padova, Italy
I. Ribas
Affiliation:
IEEC Barcelona, Catalonya, Spain
G. Tosti
Affiliation:
Dipartimento di Fisica, Università di Perugia, Perugia, Italy
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Abstract

We present the science case for ICE-T, the International Concordia Explorer Telescope, a double telescope optimized for ultra-high and ultra wide field optical time-series photometry from Dome C. ICE-T consists of two 60 cm 8°×8°-FOV Schmidt telescopes for Sloan g and i photometry and one independent 25 cm, solar, full-disk, Ca ii-K imaging telescope on a single mount. ICE-T is therefore operable during night and day. A 28 cm narrow-field Maksutov spectrophotometric telescope for night-time aerosol measurements (TAVERN-SP) will be provided by AWI early on and operated in parallel with IRAIT and later with ICE-T. The low scintillation noise and the long continuous darkness are among the unique properties for high precision optical time-series photometry.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

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