Visualization Project Seeing and Hearing the CMB.
Cosmological Structure Formation A Short Course II. The Growth of Cosmic Structure Chris Power.
Cosmic Acceleration 1)The evidence 2)What it could be 3)Why each options is interesting/confusing 4)Planning the next steps.
CMB constraints on WIMP annihilation: energy absorption during recombination Tracy Slatyer – Harvard University TeV Particle Astrophysics SLAC, 14 July.
Analysis of NuSTAR Bkg Analysis of NuSTAR Bkg Fabio Gastaldello & Silvano Molendi (IASF-Milano/INAF) 1.
Astro-2: History of the Universe Lecture 11; May 21 2013.
CMB Anisotropy & Polarization in Multiply Connected Universes
Cosmology Basics. We see photons today from last scattering surface when the universe was just 400,000 years old The temperature of the cosmic microwave.
Atomic Precision Tests and Light Scalar Couplings Philippe Brax IPhT Saclay « The Proton Radius Puzzle » Workshop, Trento November 2012 P.B and C. Burrage,
ALMA and the Formation of Galaxies Pierre Cox IAS, Orsay, France.
What have we learnt from WMAP?
History of cosmic web of galaxies History of cosmic web of galaxies Agnieszka Pollo Laboratoire d'Astrophysique de Marseille (LAM) Marseille, France.
