The Cosmic Lens All-Sky Survey parent population - I. Sample selection and number counts


A major source of uncertainty in the analysis of gravitational-lens surveys is the distribution in the redshift-luminosity plane of the population to which the lensed sources belong. This is a step to reduce this uncertainty.

This is a pre-copyedited, author-produced version of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record is available at the URLs mentioned on the abstract page, in my publication list, and at the basic-information page for this work.

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