Constraints on H_0 from combining CMB, Large Scale Structure, Supernovae and Clusters

Details Constraints on H_0 from combining CMB, Large Scale Structure, Supernovae and Clusters Constraints on H_0 from combining CMB, Large Scale Structure, Supernovae and Clusters

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.144l&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Cosmic Microwave Background provides one of the most promising routes for determination of the cosmological parameters. In conjunction with information from large scale clustering, supernovae distances and galaxy clusters, it is already possible to put interesting constraints on H_0. These will be discussed, along with the substantial improvements expected from the next generation of CMB data from ground, balloon and satellite-based experiments.

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