Conference aims


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.