Nanjing, March 2003 Using the Sunyaev-Zeldovich effect to probe the gas in clusters Mark Birkinshaw University of Bristol.
(Radio) Astronomy in Taiwan Jeremy Lim Institute of Astronomy & Astrophysics, Academia Sinica (ASIAA), Taiwan Taiwan (22.5 million) Malaysia (23 million)
WRIGHT - Cosmology Tutorial
CfA Oct 8 2003 Determining the Cosmic Distance Scale with Galaxy Clusters Erik Reese University of California, Berkeley.
K.S. Dawson, W.L. Holzapfel, E.D. Reese University of California at Berkeley, Berkeley, CA J.E. Carlstrom, S.J. LaRoque, D. Nagai University of Chicago,
High Resolution Observations of the CMB with the CBI Interferometer XVIII th IAP Colloquium - July 1 2002 Carlo Contaldi CITA.
(Eisenstein et al., ApJ, 2005) Surveys of large scale structure will probe Dark Energy by measuring the BAO scale vs. redshift. Planned: DESI, Euclid,
KEY EVIDENCE RELEVANT TO THE STANDARD MODEL Observation Verdict Extra Yes NoAssumption CMB Acoustic Peaks X Baryon Acoustic Peak X Cold Dark Matter Type.
Clusters of Galaxies in the Microwaves
The KAT/SKA project and Related Research Catherine Cress (UKZN/KAT/UWC)
Correlation of GRB and CMB peaks ( view from the CMB frame )
Galaxies, Cosmology and the SKA Catherine Cress (UWC)
