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Figure 1:
The temperature power spectrum for the best-fit
power-law ![]() ![]() ![]() ![]() |
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Figure 2: Velocity versus luminosity-distance for type Ia supernovae (filled circles), S-Z clusters (open circles) and gravitational lens time-delay systems (filled triangles), with z>0.05. All curves shown correspond to flat models and are labelled with the Hubble parameter in km s-1 Mpc-1. |
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Figure 3:
CMB angular power spectra for models with
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Figure 4:
The temperature power spectrum for the best-fit
power-law ![]() ![]() ![]() ![]() |
Open with DEXTER |
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Figure 5:
The temperature-polarization (TE) cross
power-spectrum and the polarization (EE) power spectrum for our E-deS
models with
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Figure 6:
The power spectrum of large scale structure
at z=0 and z=2.3 for our E-deS models with
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