| POSTERS | |
| S.Ansari : | The significance of wavelength coincidence statistics in abundance determination within the context of GAIA | 
| I.Busa` : | NLTE line-blanketed CaII IRT calculation for evaluation of GAIA spectroscopic performances | 
| M.Cropper : | GAIA spectroscopy and the mass ratios in cataclysmic variables | 
| E.Grebel : | An extragalactic reference frame for GAIA and SIM using SDSS QSOs | 
| A.Kucinskas : | AGB stars as tracers of star formation histories: implication for GAIA photometry and spectroscopy | 
| T.Lejeune : | Compared photometric properties of stellar atmosphere models for cool stars | 
| P.Marrese : | GAIA spectroscopy of symbiotic binaries | 
| P.Marrese : | Expanding the sample of real spectra of cool stars for GAIA | 
| E.F.Milone : | GAIA and the boon to extrasolar planet studies | 
| P.Niarchos : | Evaluating the GAIA performance on the photometry of eclipsing binaries: the case of near-contact and contact binaries | 
| A.Niedzielski : | H/He ratio in WR stars | 
| M.Odenkirchen : | The extended tidal tails of Palomar 5: tracers of the Galactic potential | 
| M.Paparo : | Missing spectroscopy of Theta Tucanae | 
| Y.Pavlenko : | GAIA spectroscopy of Carbon stars | 
| A.Prsa : | Automated coarse computation of parameters of eclipsing binaries | 
| S.Ragaini : | GAIA spectroscopy of active solar-type stars | 
| A.Rosenbush : | Some results of the monitoring of the IR triplet Ca II lines profiles in stars with the R Coronae Borealis type variability | 
| F.Royer : | Spectroscopy with FLAMES: applications to GAIA RVS | 
| J.Skuljan : | A detailed analysis of the precision of stellar radial velocities obtained using the HERCULES spectrograph | 
| R.Tantalo : | Line indices as age, metallicity and abundance indicators | 
| G.Wahlgren : | Atomic data for the GAIA spectral wavelength region | 
| P.Willemsen : | Derivation of stellar parameters from DIVA spectral data | 
| T.Zwitter : | Crowding in the GAIA spectrograph focal plane | 
| T.Zwitter : | Information recovery from overlapping GAIA spectra |