New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies

We present neutrino mass bounds using 900,000 luminous galaxies with photometric redshifts measured from Sloan Digital Sky Survey III Data Release Eight (SDSS DR8). The galaxies have photometric redshifts between $z=0.45$ and $z=0.65$, and cover 10,000 square degrees and thus probe a volume of 3$h^{-3}$Gpc${}^3$, enabling tight constraints to be derived on the amount of dark matter in the form of massive neutrinos. A new bound on the sum of neutrino masses $\sum m_{\nu }<0.26$ eV, at 95% confidence level (CL), is obtained after combining our sample of galaxies, which we call “CMASS”, with WMAP 7 year Cosmic Microwave Background (CMB) data and the most recent measurement of the Hubble parameter from the Hubble Space Telescope (HST). This constraint is obtained with a conservative multipole range choice of $30 < \ell < 200$ in order to minimize non-linearities, and a free bias parameter in each of the four redshift bins. We study the impact of assuming this linear galaxy bias model using mock catalogs, and find that this model causes a small ($\sim 1-1.5 \sigma$)biasin$\Omega_{\rm DM} h^2$. For this reason, we also quote neutrino bounds based on a conservative galaxy bias model containing additional, shot noise-like free parameters. In this conservative case, the bounds are significantly weakened, e.g. $\sum m_{\nu }<0.36$ eV (95% confidence level) for WMAP+HST+CMASS (${\mathrm{\ell }}_{\mathrm{m}\mathrm{a}\mathrm{x}}=200$). We also study the dependence of the neutrino bound on multipole range (${\mathrm{\ell }}_{\mathrm{m}\mathrm{a}\mathrm{x}}=150$ vs $\ell_{\rm max}=200$) and on which combination of data sets is included as a prior. The addition of supernova and/or Baryon Acoustic Oscillation data does not significantly improve the neutrino mass bound once the HST prior is included. [abridged]