Lensing statistics gives a method of testing the cosmological constant at
intermediate redshifts---at low and high redshifts the possibilities for
measuring $\lambda_{0}$ are limited and even at intermediate redshifts
$\lambda_{0}$ often cancels out in observable relations---using well-understood
lens theory and standard astrophysical assumptions
info and local links to full
paper
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doi:10.1111/j.1749-6632.1995.tb17617.x
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ADS: 1995NYASA.759..600H
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