Working Groups
| Function | Contributing Groups | Coordinators |
|---|---|---|
| Survey Overview | Co-PIs | Gilmore, Randich |
| Management Overview | Steering Group | 12 members |
| Paranal Observations | WG0: ESO, Lund, MPiA, Padova | T. Bensby (Se) |
| Target selection, Calibrators, FPOSS & OBs | ||
|
Open Clusters: membership analysis auxiliary data target selection |
WG1, 2, 4: Alicante, Armagh, Torino, ETH, MSSL, Vienna, MPIA, Palermo, Barcelona, Granada, Bologna, Madrid (CAB), ESO, ESA, Geneva, AIP Herts, Arcetri, Uppsala, RO Belg, Leicester, Indiana, Graz, Lisbon, Grenoble, Keele, IAC, Athens, Exeter, Birmingham, Padova, Catania, Porto, Nice, ZAH |
E. Alfaro (Sp) E. Paunzen (At) A. Bragaglia (I) |
| Galactic Plane & Field Selection | WG3: Cambridge, ZAH, ANU, MPIA, Paris, RUG, AIP, MSSL, Strasbourg, Oxford | C. Babusiaux (Fr) |
| Calibrators & Standards | WG5: AAO, AIP, Uppsala, Cambridge, Bordeaux, Antwerp, Bologna, Madrid, Paris, MPA, ANU | E. Pancino (I) |
|
OB/FPOSS generation: Field Survey Cluster Survey |
WG6: Paris, ESO, Cambridge, Lund, AIP, ZAH, Arcetri, Bologna, Catania, Padova, Palermo, IAC, Exeter, Alicante, CAUP, ESO |
T. Bensby (Se) E. Flaccomio (I) |
| Spectrum Extraction Pipelines | ||
|
Pipeline Raw Data: GIRAFFE Reduction UVES Reduction |
WG7: CASU, Keele Arcetri |
M. Irwin (UK) L. Morbidelli (I) |
| Radial Velocities | WG8: Cambridge, Keele, Arcetri, Antwerp, ZAH | Cambridge/Keele/Arcetri |
| Discrete Classification | WG9: Cambridge, MPIA, IAC, Madrid, MSSL, Porto, ZAH | S. Koposov (UK) |
| Spectrum analyses | ||
|
FGK Stars: GIRAFFE incl QC |
WG10: Paris, MPA, Lund, Uppsala, Nice, Bordeaux, Arcetri, Bologna, Liège, Geneva, Alicante, Nice, ESO, Porto, ZAH, Arcetri, Naples, Catania, Padova, Kaypten, IAC, ANU | A. Recio-Blanco (Fr) & C. Allende Prieto (Sp) |
|
FGK Stars: UVES incl QC |
WG11: Paris, MPA, Lund, Uppsala, Nice, Vilnius, Arcetri, ANU, Bologna, AIP, Indiana, UCM, Herts, Groningen, ESO, Naples, Porto, Catania, Alicante, Padova, Liège, Bordeaux, ZAH, IAC, Chile | A. Korn (Se) & R. Smiljanic (ESO) |
| WG10/11 Interface | Recio-Blanco, Allende Prieto, Pasquini, Smiljanic, Korn, Hill | |
| Pre-Main-Sequence stars incl QC | WG12: Arcetri, Catania, IAA, Naples, Palermo, ETH, CAUP, Keele, Exeter, Madrid (UCM, CAB) | A. Lanzafame (I) |
| OBA Stars incl QC | WG13: Liège, RO Belg, AIP, IAC, OMA, Madrid, Paris, Alicante, Uppsala, MPIA, ZAH, Leuven, Herts, Calar Alto, Nice, IAA, IAC, Armagh | R. Blomme (Be) |
| Unusual Objects incl QC | WG14: SRON, Nijmegen, Warwick, IAC, Leuven MPIA, Herts, IAC, ZAH | S. van Eck (Be) |
| Quality Control, Parameter Homogenization | ||
| Survey Parameter Homogenisation | WG15 & WG5: all spectrum analysis groups | P. Francois (Fr) |
| Survey monitoring, database, archive | ||
| Survey Progress | WG16: CASU | Co-PIs |
| Operational database & Phase 3 | WG17: CASU/Cambridge | CASU |
| Survey Archive | WG18: AIP, RUG, Madrid, Vienna, ZAH, Edin | N. Hambly (UK) |
| Outreach | WG19: Cambridge | N. Walton (UK) |
Page last updated: 19/03/2013
