Home List of Titles WiggleZ Dark Energy Survey: cosmological neutrino mass constraint from blue high-redshift galaxies
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/222873
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- WiggleZ Dark Energy Survey: cosmological neutrino mass constraint from blue high-redshift galaxies
- Riemer-Sorensen, Signe; Blake, Chris; Parkinson, David; Davis, Tamara M.; Brough, Sarah; Colless, Matthew; Contreras, Carlos; Couch, Warrick; Croom, Scott; Croton, Darren; Drinkwater, Michael J.; Forster, Karl; Gilbank, David; Gladders, Mike; Glazebrook, Karl; Jelliffe, Ben; Jurek, Russell J.; Li, I-hui; Madore, Barry; Martin, D. Christopher; Pimbblet, Kevin A.; Poole, Gregory B.; Pracy, Michael; Sharp, Rob; Wisnioski, Emily; Woods, David; Wyder, Ted K.; Yee, H. K. C.
- The 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 ∑mν<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 ∑mν<0.29 eV, which is the strongest neutrino mass constraint derived from spectroscopic galaxy redshift surveys.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Physical Review D: Particles, Fields, Gravitation and Cosmology, Vol. 85, no. 8 (Apr 2012), article no. 081101
- Publication year
- FOR Code(s)
- 0201 Astronomical and Space Sciences; 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics; 0206 Quantum Physics
- Blue galaxies; Cosmology; High-redshift galaxies; Neutrino mass
- American Physical Society
- Publisher URL
- Copyright © 2012 American Physical Society. The published version is reproduced with the kind permission of the publisher.
- Research Projects
- Full text
- Peer reviewed