Wp1000 | Management |
Wp2000 | Spectrometric, photometric and astrometric reduction |
| Wp2100 | Photometry and astrometry in the in-plane bulge region |
| Wp2200 | Spectroscopic reduction of the bar |
| Wp2300 | Spectroscopic reduction of the inner disc |
| Wp2400 | Spectroscopic reduction of the inner thick disc |
| Wp2500 | Spectroscopic reduction of the outer thick disc |
| Wp2600 | Abundance analysis methodologies: inter-comparisons,homogeneity |
Wp3000 | Dynamical modelling |
| Wp3100 | Made-to-measure method implementation |
| Wp3200 | Ready-to-wear chemo-dynamic method implementation |
Wp4000 | Direct chemo-kinematic interpretation |
| WP4100 | Bulge-bar-disc connection |
| | Wp4110 | Structure and kinematics of the bulge region |
| | Wp4120 | Understanding the bulge/bar/disc connection through chemo-dynamics |
| Wp4200 | Radial structure of the disc |
| Wp4300 | Vertical structure of the disc |
Wp5000 | Global modelling and interpretation of the bulge-bar-disc system |
| Wp5100 | Population synthesis model |
| Wp5200 | Made-to-Measure approach |
| Wp5300 | Ready-to-wear approach |
| Wp5400 | Galactic dynamics:synthesis and conclusions |