Lecture plan: Part 1 (Smooth Universe)
10+1 lectures

Lec 1  - Overview
Lec 2  - Hubble + FLRW [Brief history of Hubble & Lemaitre; Hubble’s law; FLRW metric]
Lec 3  - Kinematics [Light propagation & redshift; luminosity dist; angular diam dist; Cosmography]
Lec 4  - Kinematics [K-correction; source counts; geodesic motion; BB radn]
Lec 5  - Dynamics [Friedmann eqns; solutions of Friedmann eqns; age of universe; horizons; critical density]
Lec 6  - Standard model [energy components - radiation (CMBR obsvn), baryons, dark matter (+evidence:vir thm, rotn curves, CMB), Lambda/dark energy (+evidence), curvature=0 (+evidence)]
Lec 7  - Thermal history [distribution funcs in FLRW; relativ and non-relativ species in equilib; counting relativistic degrees of freedom]
Lec 8  - Thermal history [entropy; decoupling: distributions after decoupling, neutrinos]
Lec 9  - Thermal history [decoupling: recombination, WIMPS; BBN]
Lec 10 - Inflation & scalar fields
Lec 11 - Important epochs [a_eq; a_lastscat; a_Lambda]  
       -  Alternatives to standard model [steady state+; MOND+; mod grav+; backreaction]

Lecture plan: Part 2 (Inhomogenous Universe)

Lec 12 - Relativistic linear perturbation theory [perturbed quantities, gauge invariance]
Lec 13 - Relativistic linear perturbation theory (contd) [resulting equation, evolution as a function of k, transfer function]
Lec 14 - Transfer function, Newtonian linear perturbation theory [equations]
Lec 15 - Newtonian perturbation for DM, baryons, Jeans scale
Lec 16 - Zeldovich approximation, Spherical collapse
Lec 17 - Statistical quantities: power spectrum
Lec 18 - Velocity field, RSD
Lec 19 - Mass function, excursion sets
Lec 20 - Galaxy clustering, bias
Lec 21 - Baryons, galaxy formation