The Structure Formation Cookbook 1. Initial Conditions: A Theory for the Origin of Density Perturbations in the Early Universe Primordial Inflation: initial.
The physics of inflation and dark energy 1.3 Dark energy: some evidence (short list) Ages of glob. clusters/galaxies at z~2-3: m 0.6 SN Ia: -
Sami Dib NBI, STARPLAN Unveiling the diversity of the MW stellar clusters + Sacha Hony (ITA/Heidelberg) Stefan Schmeja (ARI/ Heidelberg) Dimitrios Gouliermis.
A Survey for Large Separation Lensing Among 9100 FIRST Quasars
NGC4603 Cepheids in NGC4603 Planetary Nebula Luminosity Function Number.
Selecting a mass function by way of the Bayesian Razor Darell Moodley (UKZN), Dr. Kavilan Moodley (UKZN), Dr. Carolyn Sealfon (WCU)
The Initial Mass Function in Clusters
Weak-Lensing selected, X-ray confirmed Clusters and the AGN closest to them
Selecting a mass function by way of the Bayesian Razor
