The Homogeneous Universe 
03: The zeroth order Universe 
04: The metric and its degrees of freedom 
05: The cosmological fluid
06: The background evolution

The Inhomogeneous Universe
07: The density contrast random field
08: Statistical properties of the density contrast field
09: Parameterization of the density contrast field

Structure formation
10: Newtonian perturbed fluid equations
11: Dark matter linear clustering
12: Baryonic matter linear clustering
13: Non-linear clustering
14: Perturbations in general relativity

Cosmological probes
15: BAO and CMB
16: Galaxy clustering
17: Weak lensing

HOMEWORK

HW1
HW2
HW3
HW4