Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig1.eps}\end{figure}$ Figure 1: The 68, 95, and $99\%$ confidence contours arising from fitting the CMBR shift parameter. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha=-4.38,\ \protect\beta=0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig2.eps}\end{figure}$ Figure 2: The 68, 95, and $99\%$ confidence contours arising from fitting the SN Ia data. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig3.eps}\end{figure}$ Figure 3: The combined 68, 95, and $99\%$ confidence contours arising from fitting the SN Ia and the CMBR shift parameter data. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig4.eps}\end{figure}$ Figure 4: The 68, 95, and $99\%$ confidence contours arising from fitting the length scale associated with the baryon oscillations. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig5.eps}\end{figure}$ Figure 5: The 68, 95, and $99\%$ confidence contours arising from fitting the combined data from the SNIa, CMBR shift parameter and the length scale associated to the baryon oscillations. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig6.eps}\end{figure}$ Figure 6: The 68, 95, and $99\%$ confidence contours arising from fitting the linear growth factor using the spherical collapse approach. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig7.eps}\end{figure}$ Figure 7: The 68, 95, and $98\%$ confidence contours arising from fitting to the Combined SNIa, shift parameter, baryon oscillations and the linear growth data sets. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig1.eps}\end{figure}$	Figure 1: The 68, 95, and $99\%$ confidence contours arising from fitting the CMBR shift parameter. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha=-4.38,\ \protect\beta=0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig2.eps}\end{figure}$	Figure 2: The 68, 95, and $99\%$ confidence contours arising from fitting the SN Ia data. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig3.eps}\end{figure}$	Figure 3: The combined 68, 95, and $99\%$ confidence contours arising from fitting the SN Ia and the CMBR shift parameter data. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4994fig4.eps}\end{figure}$	Figure 4: The 68, 95, and $99\%$ confidence contours arising from fitting the length scale associated with the baryon oscillations. The parameter values corresponding to the concordance $\Lambda$ CDM model ( $\Omega _{\rm m}=0.27,\ \Omega _{\Lambda }=0.73$ or $\alpha =-4.38,\ \beta =0$ ) are marked with a cross. The gray area represents a section of the parameter space that is not allowed.
Open with DEXTER