of $m_{1/2}$ in the cMSSM for different $A_0$, $\tan\beta = 10$; from [@Heinemeyer:2004xw].[]{data-label="fig:cmssm"}](strip.eps "fig:"){width="4.2cm" height="4.1cm"} ![(a) The WMAP strip for $\mu > 0$, $A_0 = 0$ and $\tan\beta = 10$ in the cMSSM; from [@Heinemeyer:2004xw]. (b) Scatter plot of the masses of the LVSP and the NLVSP in the cMSSM; from [@Ellis:2004bx]. (c) Scatter plot of the masses $m_1$=$m_{\tilde{\chi}^0_1}$ and $m_2$=$m_{\tilde{\chi}^0_2}$ of cMSSM models satisfying $\tan\beta$ = 10, 20, 35 and $A_0=0$. (d) $\chi^2$ fits based on the current experimental EW precision observables and DM constraints as functions of $m_{1/2}$ in the cMSSM for different $A_0$, $\tan\beta = 10$; from [@Heinemeyer:2004xw].[]{data-label="fig:cmssm"}](nvsp.eps "fig:"){width="4.6cm" height="4.2cm"} ![(a) The WMAP strip for $\mu > 0$, $A_0 = 0$ and $\tan\beta = 10$ in the cMSSM; from [@Heinemeyer:2004xw]. (b) Scatter plot of the masses of the LVSP and the NLVSP in the cMSSM; from [@Ellis:2004bx]. (c) Scatter plot of the masses $m_1$=$m_{\tilde{\chi}^0_1}$ and $m_2$=$m_{\tilde{\chi}^0_2}$ of cMSSM models satisfying $\tan\beta$ = 10, 20, 35 and $A_0=0$. (d) $\chi^2$ fits based on the current experimental EW precision observables and DM constraints as functions of $m_{1/2}$ in the cMSSM for different $A_0$, $\tan\beta = 10$; from [@Heinemeyer:2004xw].[]{data-label="fig:cmssm"}](lvsp3.ps "fig:"){width="4.7cm" height="4cm"} ![(a) The WMAP strip for $\mu > 0$, $A_0 