1. Introduction
2. Data and Mock Samples
2.1. Data
2.2. Photometric Redshifts, Luminosities, and Stellar Masses
2.3. Mock Samples
3. VIPERS Density Field
4. Dependence of Stellar Mass and sSFR on the Local Density
4.1. Passive and Active Galaxies
4.2. Stellar Mass Segregation in Different Environments
4.3. sSFR as a Function of Environment
5. Comparison with the Adopted Model
5.1. R Mocks vs V Mocks
5.2. Comparison between Data and R Mocks
6. Discussion
6.1. VIPERS in Context
6.2. Insights from the Model
7. Summary and Conclusions