1
Syllabus
2
Introduction: Main events in the evolution of the Universe
3
Rotation of Spiral galaxies
4
Surface Brightness of Spiral galaxies
5
Barred galaxies
6
Elliptical galaxies
7
Milky Way galaxy
8
Local Group
9
Galaxy Luminosity function
9
Evolution of Galaxy Luminosity function
10
Large-scale distribution of galaxies
11
Clustering of galaxies: power spectrum and correlation function
13
Mid term Exam
14
Kinematics of particles.Elements of cosmology: Friedmann Equation
15
FRW metric. Horizon. Distances.
16
Elements of cosmology: Friedmann Equation
17
Growth of perturbations: Modes, waves longer than horizon.
18
Linear Growth of perturbations I: waves shorter than horizon.
19
Linear Growth of perturbations II
20
Transfer Functions
21
Halo Mass Function
22
Zeldovich Approximation
23
Halo properties
25
Galaxy formation.
26
Galaxies at high z I
27
Galaxies at high z II
28
Galaxies at high z III
29
COSMOparticle: Linear growth of fluctuations
30
COSMOparticle: Non Linear growth. Biases. Distortions.
31
COSMOparticle: connecting DM and light.
32
COSMOparticle: halo abundances. Overabundance problems..
33
COSMOparticle:Properties of DM halos: structure and evolution.
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Review
Useful Links
Ned Wright's cosmology Tutorial
Wayne Hu cosmology class
Eisentein,Hu transfer functions