from preparation to support and follow-up

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Presentation transcript:

from preparation to support and follow-up Programme 1: monitoring photometric variability of delta Scuti, gamma Dor, beta Cep, candidate COROT targets (SPM, ESO) : PI: Poretti, with distribution of tasks as discussed by Ennio Programme 2: radial velocity and line profile variations of delta Scuti, gamma dor, beta Cep observed by COROT (= large programme?) : PI: Poretti Programme 3: monitoring photometric and spectroscopic variability of Be star, candidate COROT targets (FEROS, LNA, OHP + Espadons/Narval, OSN) : PI: Neiner et al. Programme 4: magnetic activity of COROT targets (Espadons @ CFHT, Narval @ TBL) : PI: Catala et al. Programme 5: seismology with Harps (ESO 3.6m) PI: Mosser et al. Programme 6: diameters via interferometry (AMBER @ VLTI) PI: Schmider et al.

Overall strategy 1: large programme at ESO: FEROS - Vrad and LPV for dScuti, gDor, bCep, Be 2: large programme at OHP: Sophie - Vrad and LPV for dScuti, gDor, bCep, Be 3: large programme at TBL: Narval - magnetic field, activity and LPV for F,G-type, Be stars 4: (smaller) programme - seismology of solar-type stars with Harps (ESO 3.6m) 4b: programme - seismology of solar-type stars with SOPHIE (OHP) 5: diameters via interferometry (AMBER @ VLTI)