The K-band luminosity function of nearby field galaxies
Abstract
We present a measurement of the K-band luminosity function (LF) of field galaxies obtained from near-infrared imaging of a sample of 345 galaxies selected from the Stromlo-APM Redshift Survey. The LF is well-fitted over the ten magnitude range -26 < M_K < -16 by a Schechter function with parameters alpha = -1.16 +- 0.19, M* = -23.58 +- 0.42, phi* = 0.012 +- 0.008 Mpc^-3 assuming a Hubble constant of H_0 = 100 km/s/Mpc. We have also estimated the LF for two subsets of galaxies subdivided by the equivalent width of the Halpha emission line at EW(Halpha) = 10A. There is no significant difference in LF shape between the two samples, although there is a hint (~1 sigma significance) that emission line galaxies (ELGs) have M* roughly one magnitude fainter than non-ELGs. Contrary to the optical LF, there is no difference in faint-end slope alpha between the two samples.
Keywords
Cite
@article{arxiv.astro-ph/9907179,
title = {The K-band luminosity function of nearby field galaxies},
author = {Jon Loveday},
journal= {arXiv preprint arXiv:astro-ph/9907179},
year = {2009}
}
Comments
10 pages, 9 embedded figures, MNRAS, in press. Minor changes to correspond to accepted version