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A Search for Cosmic Microwave Background Anisotropies on Arcminute Scales

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Figure

Figure 1.1: Hubble’s velocity versus distance relation for extra-galactic nebulae. Figure taken from Hubble [66].
Figure 1.4: Current measurements of the CMB power spectrum, including data from the WMAP three-year release [63], the 2003 flight of BOOMERANG [69], and ACBAR [78]
Figure 1.6: The thermal and kinetic SZE distortions of the CMB caused by a typical massive cluster with y = 10 −4 , k B T e = 10 4 keV, and v
Figure 1.7: Examples of the dependence of two SZE observables as a function of some of the cosmological parameters
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