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\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Figure 1 (Left): Projected 68\% statistical confidence intervals on the dark energy equation of state possible from {\it  SNLS} when it is completed 5 years from now, assuming a flat universe (from CMB measurements), and with (black-solid) and without (blue-dash) a prior of $\Omega _M$ from Large-Scale Structure. If a small systematic error is introduced, the statistical confidence interval will miss the correct, $\Lambda $ solution by $2\sigma $. Figure 2 (Right): The stretch-corrected SNe\nobreakspace  {}Ia Hubble diagram for the SCP dataset plotted according to the class of the host galaxy. The inset shows the high-redshift SNe, the main panel the Hubble diagram for the entire sample. SNe\nobreakspace  {}Ia in E/S0 host galaxies show significantly less scatter than those in later types, and the two types agree (Sul03). }}{4}}
\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces  CMAGIC CAPTION. one will be B-I, other will be B-V. }}{5}}