Conference's goals include: |
review of science goals for GAIA spectroscopy, |
| foreseeable achievements by GAIA spectroscopy, |
| outline of spectrograph design and involved technology, |
| telemetry and compression algorithms, |
| synergy with GAIA photometry and astrometry, |
| legacy to ground-based spectroscopy, |
| tools for spectral data analysis and treatment, |
| wavelength and flux calibration of GAIA spectra, |
| automatic data treatment and measurement. |
Topics to be discussed: |
radial and rotational velocities, |
| astrometric radial velocities, |
| derivation of stellar atmospheric parameters (Teff, log g, micro-turb., ...), |
| stellar atmospheric models (Kurucz, MARCS, Phoenix,...), |
| chemical abundance analysis and atomic constants, |
| spectral peculiarities of various kind, |
| signature of mass loss and interstellar medium, |
| stellar pulsation, |
| binarity and eclipsing stars, |
| spectral classification over the GAIA wavelength region, |
| Galaxy kinematics, structure and evolution from GAIA spectroscopy, |
| stellar structure and evolution from GAIA spectroscopy, |
| support to extra-solar planets and foundamental physics investigations. |