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A wide-field K-band survey. The luminosity function of galaxies

J. P. Gardner·R. M. Sharples·C. S. Frenk·B. E. Carrasco
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Abstract

We present the first determination of the near-infrared K-band luminosity function of field galaxies from a wide field K-selected redshift survey. The best fit Schechter function parameters are $M^* = -23.12 +5log(h)$, $α= -0.91$, and $ϕ^* = 1.66 \times 10^{-2} h^3 ~ Mpc^{-3}$. We estimate that systematics are no more than 0.1 mag in $M^*$ and 0.1 in $α$, which is comparable to the statistical errors on this measurement.

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J. P. Gardner, R. M. Sharples, C. S. Frenk, B. E. Carrasco. 1997-02-20. A wide-field K-band survey. The luminosity function of galaxies. https://doi.org/10.1086/310630

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