Instrument session

coordinator: M. Auvergne

This session is the follow-up of the session held in Vienna, and focusses on few specific topics, where new results have been recently obtained.
 

1.Mission status	L. Boisnard
2.Pointing	2.1.Results of the AOCS simulations.L. Boisnard 2.2. Effects of the jitter on the photometry and ground-based processing -in the exoplanet channel : M. Ollivier  -in the seismology channel : M. Auvergne
3.Straylight from the earth:	3.1. Present status, and prospectsA. Baglin 3.2. Efficiency of the onboard processing background measurements and correctionsM.Auvergne
4.The CCDs flight models, characteristics and new measurements	Jean-Tristan Buey et al.

Reports of the Working groups
 

*Seismology WG
 

General report	E. Michel
Corot H&H2 Results and conclusions	J. Provost, G.Berthomieu, P. Morel
The oscillations of rapidly rotating stars	M. Rieutord
Delta scuti stars as primary and secondary targets	E. Poretti et al.
Observations of bet Cep and slowly pulsating Bstars	C. Aerts
Lambda Bootis, HD 183 324	E.Pauntzen and W. Weiss

*Seismology Ground based observations WG

*Exoplanet WG
 

Work in progress and general introduction	P. Barge
Stellar classification of the COROT/Exoplanet stars	C. Moutou
Entry data of COROT/Exoplanet fields	M. Deleuil
Building the photometric masks for the exoplanet data channel	A. Llebaria
High precision radial velocity follow-up of COROT's detected transits	F. Bouchy
BEST	H. Rauer
Stellar Activity	B. Foing
Discrimination of stellar activity from planetary transits	A. Lanza
Influence of the jitter noise and its partial correction	M. Ollivier
Incidence of confusion by variable background stars	A. Leger
Scientific processing of the exoplanet channel	R. Cautain, L. Jorda
Planet detection capability of COROT	P. Borde, D. Rouan, A. Léger
A comparative study of the transit detection methods	B. Tingley
Light-curves of the "pegasides": - detection with COROT	T. Guillot

*Additional programmes WG
 

General Report

W.W. Weiss