Measurements of Omega and Lambda from 42 High-Redshift Supernovae

(Perlmutter et al, LBNL-41801, 1998, accepted for publication in Ap.J.)

(1) The matrix of numbers that represents the "Fit C" probability
distribution, plotted as confidence region contours in Figure 7, is given
here.

(2) The matrices of the small correlations of uncertainties between
the supernovae is given here.