Flux-averaging Analysis of Type Ia Supernova Data


We have combined the type Ia supernova (SNe Ia) data from the High-z SN Search and the Supernova Cosmology Project, and binned the combined data by flux-averaging in redshift intervals of ∆z = 0.05 and ∆z = 0.1. We find that the unbinned data yield a Hubble constant of H0 = 65 ± 1 km s−1 Mpc−1 (statistical error only), a matter density fraction of Ωm = 0.7… (More)


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@inproceedings{Wang1999FluxaveragingAO, title={Flux-averaging Analysis of Type Ia Supernova Data}, author={Yun F. Wang}, year={1999} }