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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{5331fig1.ps}\end{figure}$ Figure 1: Galaxy cluster mass functions. Filled circles: HIFLUGCS data (63 clusters); dashed line: best fit to HIFLUGCS data; upper solid line: predicted by concordance model ( $\Omega _{\rm m}=0.3,\sigma _8=0.9$ ), which was a very good fit to the WMAP 1st year data; lower solid line: predicted by best fit to the WMAP 3rd year data ( $\Omega _{\rm m}=0.234,\sigma _8=0.74$ ). The concordance model predicts too many (>200) clusters in the survey volume while the new cosmology predicts about the correct number. Adapted from Reiprich (2005, Fig. 10.87).
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{5331fig2.ps}\end{figure}$ Figure 2: The best fit model to the WMAP 3rd year data lies exactly at the intersection of the $\Omega _{\rm m}{-}\sigma _8$ relations from HIFLUGCS and COBE. COBE relation from Bunn & White (1997), calculated using a code provided by T. Kitayama. Adapted from Reiprich (2003).
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{5331fig3.ps}\end{figure}$ Figure 3: Quasi-mass functions estimated from luminosity function and luminosity-mass relations. Filled circles: $L_{\rm X}{-}M_{\rm tot}$ relation as measured with HIFLUGCS; open squares: normalization of this relation artificially divided by a factor of 2. The solid lines indicate the respective best fit mass functions: ( $\Omega _{\rm m}=0.22,\sigma _8=0.74$ ) and ( $\Omega _{\rm m}=0.29,\sigma _8=0.88$ ); the former result is very close to the new cosmology favored by WMAP and the latter very close to the concordance model.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{5331fig2.ps}\end{figure}$	Figure 2: The best fit model to the WMAP 3rd year data lies exactly at the intersection of the $\Omega _{\rm m}{-}\sigma _8$ relations from HIFLUGCS and COBE. COBE relation from Bunn & White (1997), calculated using a code provided by T. Kitayama. Adapted from Reiprich (2003).
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