 ![\[fig:gbeta\]Inverse temperature dependence of the continuum limit extrapolated chiral condensate for all our fermion masses. Shown is also the result obtained at $T=0$ and the result of the approximation of Ref. [@Hosotani:0000za].](gbeta_mg0.0000-syst-hosotaniHF.ps "fig:"){width="00.00000%"} ![\[fig:gbeta\]Inverse temperature dependence of the continuum limit extrapolated chiral condensate for all our fermion masses. Shown is also the result obtained at $T=0$ and the result of the approximation of Ref. [@Hosotani:0000za].](gbeta_mg0.000-syst-hosotaniHF.ps "fig:"){width="00.00000%"} ![\[fig:gbeta\]Inverse temperature dependence of the continuum limit extrapolated chiral condensate for all our fermion masses. Shown is also the result obtained at $T=0$ and the result of the approximation of Ref. [@Hosotani:0000za].](gbeta_mg0.00-syst-hosotaniHF.ps "fig:"){width="00.00000%"} ![\[fig:gbeta\]Inverse temperature dependence of the continuum limit extrapolated chiral condensate for all our fermion masses. Shown is also the result obtained at $T=0$ and the result of the approximation of Ref. [@Hosotani:0000za].](gbeta_mg0.0-syst-hosotaniHF.ps "fig:"){width="00.00000%"} ![\[fig:gbeta\]Inverse temperature dependence of the continuum limit extrapolated chiral condensate for all our fermion masses. Shown is also the result obtained at $T=0$ and the result of the approximation of Ref. [@Hosotani:0000za].](gbeta_mg0.0-syst-hosotaniHF.ps "fig:"){width="00.00000%"} 