The Sloan Digital Sky Survey (SDSS) has measured an optical luminosity func
tion for galaxies in five bands, finding 1.5-2.1 times more luminosity dens
ity than previous work. This Letter compares the SDSS luminosity density wi
th two recent determinations of the near-infrared luminosity function based
on the 2 Micron All Sky Survey data and finds that an extrapolation of the
SDSS results gives a 2.3 times greater near-infrared luminosity density.