Prsentation PowerPoint

1
Introduction from preparation to follow-up

• Past and Present Preparation of COROT seismology
  programme
• Stromgren photometry and high resolution
  spectroscopy of COROT potential targets
• . about 1500 stars down to mV8
• . about 400 fainter stars in the vicinity of
  primary targets
• . all data available in Gaudi database
• . data mainly used to determine fundamental
  parameters
• . resulting parameters available in Corotsky and
  Gaudi
• - G/B photometric and spectroscopic monitoring of
  some ? Scuti, ??Doradus, ? Cep and Be stars
• Future Support and follow-up of COROT seismology
  programme
• further observations of COROT targets.
• much less targets
• much more observations for each target

2
Groundbased observations in support and follow-up
of COROT seismology programme
Part 1 the current programmes (1 hour) -
introduction the existing data, Gaudi, Corotsky
(Catala, 5 min) - the status of the photometric
and spectroscopic observations of the Gamma Dor,
Delta Sct and Beta Cep targets (Poretti, 15
min) - the status of the photometric and
spectroscopic observations of Be stars
(Guttierez-Soto Hubert, 15 min) - magnetic
activity of COROT targets (Catala, 10
min) General discussion (moderator Poretti, 15
min). Specific points - do we all agree to
continue ? New observations ? - management of
available and future data ? - PI for each star
/ each programme Part 2 future Large
Programmes (1.5 hour) - The ESO Large
programme on Beta Cep, Gamma Dor, Delta Sct.
(Poretti, 15 min) Definition of the structure
and alternatives if rejected (General
discussion, moderator Catala 30 min) - New
potential Large Programmes Seismology with
HARPS on solar-like stars (Mosser, 10 min)
Seismology with SIAMOIS at Dome C (Mosser, 15
min) Measuring diameters and rotation with
AMBER (Catala 10 min) General discussion
(10 min)