Add to ORKGThe absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The WiggleZ high redshift, star-forming, and blue galaxy sample offers a complementary data set to previous surveys for performing these measurements, with potentially different systematics from nonlinear structure formation, redshift-space distortions, and galaxy bias. We obtain a limit of ∑m_ν<0.60 eV (95% confidence) for WiggleZ+Wilkinson Microwave Anisotropy Probe. Combining with priors on the Hubble parameter and the baryon acoustic oscillation scale gives ∑m_ν<0.29 eV, which is the strongest neutrino mass constraint derived from spectroscopic galaxy redshift surveys
We present here bounds on neutrino masses from the combination of recent Planck cosmic microwave bac...
We place the most robust constraint to date on the scale of the turnover in the cosmological matter ...
We investigate the cosmological implications of the latest growth of structure measurement from the ...
The absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The Wigg...
The absolute neutrino mass scale is currently unknown, but can be constrained from cosmology. We use...
The absolute neutrino mass scale is currently unknown, but can be constrained from observations of t...
We present cosmological upper limits on the sum of active neutrino masses using large-scale power sp...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
We examine whether future, nearly all-sky galaxy redshift surveys, in combination with CMB priors, w...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
We present the strongest current cosmological upper limit on the neutrino mass of ∑mν<0.18 eV (95% ...
Laboratory experiments measuring neutrino oscillations indicate small mass differences between diffe...
We place the most robust constraint to date on the scale of the turnover in the cosmological matter ...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We present here bounds on neutrino masses from the combination of recent Planck cosmic microwave bac...
We place the most robust constraint to date on the scale of the turnover in the cosmological matter ...
We investigate the cosmological implications of the latest growth of structure measurement from the ...
The absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The Wigg...
The absolute neutrino mass scale is currently unknown, but can be constrained from cosmology. We use...
The absolute neutrino mass scale is currently unknown, but can be constrained from observations of t...
We present cosmological upper limits on the sum of active neutrino masses using large-scale power sp...
We report one of the most accurate measurements of the three-dimensional large-scale galaxy power sp...
We examine whether future, nearly all-sky galaxy redshift surveys, in combination with CMB priors, w...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviole...
We present the strongest current cosmological upper limit on the neutrino mass of ∑mν<0.18 eV (95% ...
Laboratory experiments measuring neutrino oscillations indicate small mass differences between diffe...
We place the most robust constraint to date on the scale of the turnover in the cosmological matter ...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We measure the imprint of baryon acoustic oscillations (BAOs) in the galaxy clustering pattern at th...
We present here bounds on neutrino masses from the combination of recent Planck cosmic microwave bac...
We place the most robust constraint to date on the scale of the turnover in the cosmological matter ...
We investigate the cosmological implications of the latest growth of structure measurement from the ...