A simple tool for assessing the completeness in apparent magnitude of magnitude-redshift samples

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Abstract

A new tool is proposed for finding out the completeness limit in apparent magnitude of a magnitude-redshift sample. The technique, closely related to the statistical test proposed by Efron & Petrosian, presents a real improvement compared to standard completeness tests. Namely, no a priori assumptions are required concerning the redshift-space distribution of the sources. It means in particular that neither the clustering nor the evolution of the mean number density of the galaxies affects the result of the search.

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Rauzy, S. (2001). A simple tool for assessing the completeness in apparent magnitude of magnitude-redshift samples. Monthly Notices of the Royal Astronomical Society, 324(1), 51–56. https://doi.org/10.1046/j.1365-8711.2001.04078.x

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