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Fig 21.12.

Balloon (BOOMERANG) measurements of smaller-scale anisotropies. (a) This image is almost 1800 square degrees, with the false color the same as in Fig. 21.11. (b) Models of fluctuations for different geometries of the universe. (c) Relative intensities of the fluctuations on various scales. (d) We see how the BOOMERANG data fit into various other constraints on various cosmological parameters. [The BOOMERANG Collaboration]

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