Astronomy & Astrophysics

$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig1.eps}}\end{figure}$ Figure 1: The deceleration parameter q as a function of the dimensionless comoving time Ct. The present age of the universe is Ct_R=1.21 and the acceleration commences at comoving time $Ct_{\rm T}=0.66$ (cf. Sect. 5).
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In the text

$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig4.eps}}\end{figure}$ Figure 4: The dependence of the transfer function $\Delta _{\rm SW}$ on the distance traveled by the photon from the event of last scattering. The decoupling can be taken to occur at $Ct_{\rm dec}=0$ within the error bar. Reception is indicated at $Ct_{\rm R}=1.21$ .
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In the text

$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig1.eps}}\end{figure}$	Figure 1: The deceleration parameter q as a function of the dimensionless comoving time Ct. The present age of the universe is Ct_R=1.21 and the acceleration commences at comoving time $Ct_{\rm T}=0.66$ (cf. Sect. 5).
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig2.eps}}\end{figure}$	Figure 2: The relatively decreasing and growing contributions to the density contrast.
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig3.eps}}\end{figure}$	Figure 3: Time dependence of J.
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig4.eps}}\end{figure}$	Figure 4: The dependence of the transfer function $\Delta _{\rm SW}$ on the distance traveled by the photon from the event of last scattering. The decoupling can be taken to occur at $Ct_{\rm dec}=0$ within the error bar. Reception is indicated at $Ct_{\rm R}=1.21$ .
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$\begin{figure} \par\resizebox{8cm}{!}{\includegraphics{1472fig5.eps}}\end{figure}$	Figure 5: The weighing function of the ISW effect.
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