1. Tracers of the oldest Milky Way fossil records and Halo Assembly; 2. Disentangling mixed populations in the central regions of the Milky Way; 3. Galactic disks – chemodynamical properties and models; 4. Towards ages: Gaia DR1, asteroseismology, and precise abundances; 5. Stellar evolution models and stellar yields; 6. Milky Way potential and disk dynamics; 7. Cosmological simulations of Milky-Way-like galaxies; 8. Challenges in data and modeling; 9. Future outlook.