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Table 2
Summary of the analysis methodologies used by each Node involved in WG11.
| Node | Contact | Codes | Type of method |
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| Bologna | E. Pancino | DAOSPEC and GALA | Equivalent widths |
| Catania (OACT) | A. Frasca | ROTFIT | Library of observed spectra |
| CAUP | S. Sousa | ARES and MOOG | Equivalent widths |
| Concepcion | S. Villanova | DAOSPEC and GALA | Equivalent widths |
| EPInArBo | L. Magrini | DAOSPEC and FAMA | Equivalent widths |
| IAC-AIP | C. Allende Prieto | FERRE | Library of synthetic spectra |
| Liège | T. Morel | GAUFRE | Equivalent widths |
| LUMBA | S. Feltzing | SGU based on SME | Synthetic spectra computed on the fly |
| Nice | V. Hill | MATISSE | Library of synthetic spectra |
| Paris-Heidelberg | L. Sbordone | MyGIsFOS | Library of synthetic spectra |
| UCM | D. Montes | ARES and StePar | Equivalent widths |
| ULB | S. Van Eck | BACCHUS | Synthetic spectra computed on the fly |
| Vilnius | G. Tautvaišien*error*ė | DAOSPEC and MOOG | Equivalent widths |
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