Wiki MaTYSSE

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====== The MaTYSSE team ======

Gathering observers & theorists from the whole community, the MaTYSSE team is well set to efficiently tackle all issues addressed by this program. More specifically, our team include specialists of all domains involved in this program, ie stellar magnetic imaging & activity, magnetospheric accretion processes, formation & evolution of low-mass stars, exoplanets & planet migration, dynamos & stellar winds.  The full team is listed in the Table below.  

^ Partner ^ Team members ^
| France | J-F Donati, E Hébrard, L Jouve, C Baruteau (IRAP, Toulouse), J Morin (LUPM, Montepellier), F Ménard, C Dougados, J Bouvier, J Ferreira, X Delfosse, X Bonfils, T Forveille (IPAG, Grenoble), I Boisse (LAM, Marseille), G Hébrard (IAP, Paris), G Chabrier (ENS, Lyon), S Brun (CEA, Saclay), A Morbidelli, A Crida (OCA, Nice) | 
| Canada | R Doyon, E Artigau, D Lafreniere (UdM, Montreal), D Bohlender, C Marois (HIA, Victoria) | 
| Brazil | SHP Alencar, G Franco (UFMG, Belo Horizonte), J Gregorio-Hetem (Sao Paulo) | 
| CFHT | C Moutou |
| Taiwan | H Takami, SY Wang, H Shang (ASIAA, Taipei), SP Lai (NTHU, Hsinchu) | 
| ESO | G Hussain | 
| Ukraine | K Grankin, S Artemenko (CAO) | 
| China | G Herczeg (NAO, Beijing), SH Gu (NAO, Kunming) | 
| UK | I Baraffe, M Browning, S Matt (Exeter), S Mohanty, Y Unruh (Imperial), M Jardine, A Vidotto, R Fares, A Cameron, SG Gregory (StAndrews), K Rice (Edinburgh) | 
| USA | A Dupree, N Brickhouse (CfA), M Romanova (Cornell), L Rebull, L Hillenbrand (Caltech)| 
| Italy | C Argiroffi, E Flaccomio (Palermo) | 
| Switzerland | A Vidotto, F Pepe, F Bouchy, C Lovis (Geneve) | 
| Portugal | P Figueira (CAUP, Porto) |
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