Samuel R. Hinton
Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraints
Hinton, Samuel R.; Kazin, Eyal; Davis, Tamara M.; Blake, Chris; Brough, Sarah; Colless, Matthew; Couch, Warrick J.; Drinkwater, Michael J.; Glazebrook, Karl; Jurek, Russell J.; Parkinson, David; Pimbblet, Kevin A.; Poole, Gregory B.; Pracy, Michael; Woods, David
Authors
Eyal Kazin
Tamara M. Davis
Chris Blake
Sarah Brough
Matthew Colless
Warrick J. Couch
Michael J. Drinkwater
Karl Glazebrook
Russell J. Jurek
David Parkinson
Professor Kevin Pimbblet K.Pimbblet@hull.ac.uk
Director of DAIM
Gregory B. Poole
Michael Pracy
David Woods
Abstract
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. We present results from the 2D anisotropic baryon acoustic oscillation (BAO) signal present in the final data set from the WiggleZ Dark Energy Survey. We analyse the WiggleZ data in two ways: first using the full shape of the 2D correlation function and secondly focusing only on the position of the BAO peak in the reconstructed data set. When fitting for the full shape of the 2D correlation function we use a multipole expansion to compare with theory. When we use the reconstructed data we marginalize over the shape and just measure the position of the BAO peak, analysing the data in wedges separating the signal along the line of sight from that parallel to the line of sight. We verify our method with mock data and find the results to be free of bias or systematic offsets. We also redo the pre-reconstruction angle-averaged (1D) WiggleZ BAO analysis with an improved covariance and present an updated result. The final results are presented in the form of Ω c h 2 , H(z), and D A (z) for three redshift bins with effective redshifts z=0.44, 0.60, and 0.73.Within these bins and methodologies, we recover constraints between 5 and 22 per cent error. Our cosmological constraints are consistent with flat ΛCDM cosmology and agree with results from the Baryon Oscillation Spectroscopic Survey.
Citation
Hinton, S. R., Kazin, E., Davis, T. M., Blake, C., Brough, S., Colless, M., Couch, W. J., Drinkwater, M. J., Glazebrook, K., Jurek, R. J., Parkinson, D., Pimbblet, K. A., Poole, G. B., Pracy, M., & Woods, D. (2017). Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraints. Monthly notices of the Royal Astronomical Society, 464(4), 4807-4822. https://doi.org/10.1093/mnras/stw2725
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 18, 2016 |
Online Publication Date | Oct 23, 2016 |
Publication Date | Feb 1, 2017 |
Deposit Date | Oct 27, 2016 |
Publicly Available Date | Oct 27, 2016 |
Journal | Monthly notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 464 |
Issue | 4 |
Pages | 4807-4822 |
DOI | https://doi.org/10.1093/mnras/stw2725 |
Keywords | Baryon Acoustic Oscillation, WiggleZ, Dark energy, Cosmology |
Public URL | https://hull-repository.worktribe.com/output/444645 |
Publisher URL | https://mnras.oxfordjournals.org/content/early/2016/10/23/mnras.stw2725.abstract |
Additional Information | This is the advance access version of an article published in: Monthly notices of the Royal Astronomical Society, 2017, v.464, issue 4. |
Contract Date | Oct 27, 2016 |
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Copyright Statement
© Oxford University Press 2017
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