1. 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 CFHT, TBL) :
PI: Catala et al.
Programme 5: seismology with Harps (ESO 3.6m)
PI: Mosser et al.
Programme 6: diameters via interferometry VLTI)
PI: Schmider et al.

2. 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 VLTI)