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| Color Figures for Use in Presentations |
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&OmegaM-&Omega&Lambda 68%, 95%, and 99.7% constraints on &OmegaM and &Omega&Lambda obtained from CMB (orange), BAO (green), and the Union Compilation (blue). &OmegaM-w 68%, 95%, and 99.7% constraints on &OmegaM and w obtained from CMB (orange), BAO (green), and the Union Compilation (blue). Binned w 68% constraints on w(z) obtained from CMB, BAO, and the Union Compilation. w is constant over each bin. Note the poor constraints on w(z > 1). Binned Hubble Diagram and Residuals Hubble Diagrams of Union Sample constructed with selection cuts and outlier rejection. Each sample is independently binned in redshift bins of 0.01. The x-axis is sqrt(redshift). Sample Construction The samples at a glance. Left to right:
Sample Diagnostics Sample summaries at a glance. Left to right:
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| Cosmology Tables-- Data to Perform Your Own Fits |
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Union Compilation Magnitude vs. Redshift Table An ASCII table with tab-separated columns: Supernova Name, Redshift, Distance Modulus, and Distance Modulus Error Covariance Matrix A 307 by 307 tab-separated ASCII-format covariance matrix, available with or without systematics. Full Table of All SNe A latex table with columns: Supernova Name, Redshift, B-Band Magnitude, Stretch, Color, Distance Modulus, Sample, Cuts Failed (if any) CosmoMC Code for Implementing Union Compilation Tar file containing the above tables with CosmoMC code for obtaining a cosmology likelihood |
| More Figures |
&OmegaM-&Omega&Lambda and &OmegaM-w With and Without Systematics 68%, 95%, and 99.7% constraints from the Union Compilation. The filled contours show statistical constraints only; the dotted contours include systematic errors. w0-wa 68%, 95%, and 99.7% constraints from the Union Compilation. The filled contours show statistical constraints only; the dotted contours include systematic errors. |
| Lightcurve Data |
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SNe Summary Table pdf version of the table containing discovery information and redshifts. Nearby 99 Lightcurves Tar file containing lightcurve data for the nine nearby SNe. Lightcurves are in SALT format. Nearby 99 Filters Tar file containing filter throughputs for each filter used with the nearby sample, as well as the "Standard" UVBRI filters. Perlmutter et al. (1999) Lightcurves Tar file containing lightcurve data for forty two SNe from Perlmutter et al. (1999). Lightcurves are in SALT format. |