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Ω0 and λ0 from galaxy and quasar clustering: cosmic virial theorem and cosmological redshift-space distortion

Yasushi Suto

astro-pharXiv:astro-ph/9609014

Abstract

I discuss two cosmological tests to determine the cosmological density parameter Ω0 the cosmological constant λ0, which make use of the anisotropy of the two-point correlation functions due to the peculiar velocity field and the cosmological redshift-space distortion.

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