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Estimates for the Luminosity Function and Selection Function of Redshift Surveys

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The Evolving Universe

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 231))

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Abstract

We present a new method to obtain a non-parametric maximum likelihood estimate of the luminosity function and the selection function of a flux-limited redshift survey. The method parameterizes the selection function as a series of step-wise power laws and allows possible evolution of the luminosity function.

We apply our estimators to the 1.2-Jy survey of IRAS galaxies. We find a far-infrared luminosity function in good agreement with previously published results.

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© 1998 Springer Science+Business Media Dordrecht

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Springel, V., Simon, D.M.W. (1998). Estimates for the Luminosity Function and Selection Function of Redshift Surveys. In: Hamilton, D. (eds) The Evolving Universe. Astrophysics and Space Science Library, vol 231. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4960-0_29

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  • DOI: https://doi.org/10.1007/978-94-011-4960-0_29

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6082-0

  • Online ISBN: 978-94-011-4960-0

  • eBook Packages: Springer Book Archive

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