Abstract
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We propose to measure the mass function of galaxies in the local
universe. We will examine 2MASS galaxies in the isophotal magnitude
range 10.50 < K < 11.25 over the available Northern sky
(|b| > 20 °). From this large, complete sample we will obtain
kinematic measurements of a randomly selected sub-sample of 450
galaxies. We will measure their kinematic properties (projected rotation
velocity and/or centreal velocity dispersion) using FAST, the 600 line
grating, and a 2 arcsec slit. We will obtain deeper JHK and
UBVRI optical photometry of the kinematically observed galaxies
with the 48" to provide accurate photometric profiles and colors.
Statistical methods will be used to correct for ths kinematic
incompleteness.
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