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The Atacama cosmology telescope: a measurement of the cosmic microwave background power spectrum at 148 and 218 ghz from the 2008 southern survey

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Figure

Figure 1. rms temperature uncertainty for one-arcminute pixels for the 148 GHz maps (top) and 218 GHz map (bottom)
Figure 3. Azimuthal weights used for binning the 148 × 148 GHz spectrum.
Figure 4. Anisotropic noise in data and simulated patches. Top: difference map of two splits in a 148 GHz data patch (left) and its 2D power spectrum (right)
Figure 7. Single- and cross-frequency spectra plotted with the conventional
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