The final programme of the conference will become available only in early May, after the selection of oral contributions.

Until then, please be reminded that the conference will run from Monday early afternoon to Friday noon, and it will cover the following topics:

Instrumentation (lessons learned, current and future facilities)

o   ESO vision

o   High-resolution and high-precision spectrographs 

o   MOS instruments

o   Instruments calibration

Analysis of stellar spectra

o   Velocimetry

o   Stellar parameters and abundances (methods)

Exoplanets

o   Status and perspectives

o   Exoplanets in open clusters

o   Effect of stellar noise (chromospheric activity)

o   Atmospheres of exoplanets

Stellar Abundances

o   Light elements (Li, Be)

o   Abundances and stellar evolution (including open clusters)

o   Abundances and chemical evolution (obs + mod)

o   Solar twins

Globular Clusters

o   Chemical characteristics

o   Formation and evolution

Fundamental physics 

o   Testing Newton-Einstein gravity with binaries

o   Fundamental constants

o   IGM properties