  We investigate whether cosmological data suggest the need for massive
neutrinos. We employ galaxy power spectrum measurements from the Sloan Digital
Sky Survey (SDSS) and the Two Degree Field Galaxy Redshift Survey (2dFGRS),
along with cosmic microwave background (CMB) data from the Wilkinson Microwave
Anisotropy Probe (WMAP) and 27 other CMB experiments. We also use the
measurement of the Hubble parameter from the Hubble Space Telescope (HST) Key
Project. We find the sum of the neutrino masses to be smaller than 0.75 eV at
2\sigma (1.1 eV at 3\sigma).
