All Figures

$\begin{figure} \par\includegraphics[width=15.4cm,clip]{figures/3680f1.ps} \end{figure}$ Figure 1: $\alpha$ 's obtained by means of Eq. (2) from A RCHEOPS and WMAP data in the fraction of the sky covered by the former experiment. In panels a)- c), filled circles, crosses and diamonds refer to the W, V and Q bands respectively. In panels d)- f), the 143 GHz and 217 GHz channel results are given by filled circles and diamonds, respectively. The colored bands display the 2- $\sigma$ confidence limit for the $\alpha$ 's: dark grey for filled circles, intermediate grey for crosses, and light grey for diamonds. Our analysis are focused on the first patch, hosting the highest projected galaxy density.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f2.ps} \end{figure}$ Figure 2: tSZ fitted amplitude, A, as a function of patch number. We only observe a significant temperature decrement (A > 0) in patch number 1.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{figures/3680f3.ps}\par\includegraphics[width=7.8cm,clip]{figures/3680f4.ps} \end{figure}$ Figure 3: The $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 32 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we overplot the best-fit tSZ computed as discussed in the text.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f5.ps}\par\includegraphics[width=7.6cm,clip]{figures/3680f6.ps} \end{figure}$ Figure 4: $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 64 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we overplot the best-fit tSZ computed as discussed in the text.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f7.ps}\par\includegraphics[width=7.6cm,clip]{figures/3680f8.ps} \end{figure}$ Figure 5: The $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 128 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we over plot the best-fit tSZ computed as discussed in the text.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f2.ps} \end{figure}$	Figure 2: tSZ fitted amplitude, A, as a function of patch number. We only observe a significant temperature decrement (A > 0) in patch number 1.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{figures/3680f3.ps}\par\includegraphics[width=7.8cm,clip]{figures/3680f4.ps} \end{figure}$	Figure 3: The $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 32 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we overplot the best-fit tSZ computed as discussed in the text.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f5.ps}\par\includegraphics[width=7.6cm,clip]{figures/3680f6.ps} \end{figure}$	Figure 4: $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 64 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we overplot the best-fit tSZ computed as discussed in the text.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{figures/3680f7.ps}\par\includegraphics[width=7.6cm,clip]{figures/3680f8.ps} \end{figure}$	Figure 5: The $\alpha$ correlation coefficient in CMB temperature units as function of frequency in GHz for patch 1 ( top panel) and patch 201 ( bottom panel) of the 128 pixel patches. The diamonds are the WMAP data points and the stars the A RCHEOPS one. In red, we over plot the best-fit tSZ computed as discussed in the text.
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