https://digitalmaine.com/legishist113/1366/thumbnail.jp

Blake, C

Brough, S

Colless, M

Couch, WJ

Davis, TM

Drinkwater, MJ

Glazebrook, K

Hinton, SR

Jurek, RJ

Kazin, E

Parkinson, D

Pimbblet, KA

Poole, GB

Pracy, M

Woods, D

English

arXiv

© 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

Pimbblet, Kevin A.

Blake, Chris

Brough, Sarah

Colless, Matthew

Glazebrook, Karl

Kazin, Eyal

Parkinson, David

Hinton, Samuel R.

Davis, Tamara M.

Couch, Warrick J.

Drinkwater, Michael J.

Jurek, Russell J.

Poole, Gregory B.

Pracy, Michael

Woods, David

University of Hull Institutional Repository

Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraints

Maine State Legislature (113th: 1986-1988)

Maine State Documents (Maine State Library)

  MAINE STATE LEGISLATURE LAW AND LEGISLATIVE REFERENCE LIBRARY Legislative History Collection 113th Legislature (1986-1988)    History and Final Disposition  LD 367 / HP0284 AN ACT to Amend the Date to Determine Age for Kindergarten Eligibility. Presented by Rep. Begley of Waldoboro; Cosponsored by Rep. Norton of Winthrop. Education Hearing 03/10/87. Leave to Withdraw Accepted 04/27/87.   Original Bill  LD 367 (113th Legis. 1987)   Analyst's Summary of Bill  LD 367   Committee Materials  Joint Standing Committee on Education ● (Available on request—please include the following citation: cf113-LD-0367.pdf)   Floor Proceedings and Debate  HOUSE, February 17, 1987 (p161-164)  ● p. 162  SENATE, February 18, 1987 (p174-177)  ● p. 175  HOUSE, April 24, 1987 (p592-594)  ● p. 593  SENATE, April 27, 1987 (p603-606)  ● p. 604   Reports and Other Related Documents  Interim Report of the Special Comm'n to Study School Entrance Age and Preschool Services (March 1988)   Cross References  Resolve 1987, c. 64 (LD 1505)   To obtain items available on request, or to report errors or omissions in this history, please contact:  Maine State Law and Legislative Reference Library 

Legislative History:  An Act to Amend the Date to Determine Age for Kindergarten Eligibility (HP284)(LD 367)

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 Omega(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 Lambda CDM cosmology and agree with results from the Baryon Oscillation Spectroscopic Survey

University of Queensland eSpace

Repository@Hull - Worktribe

Samuel R. Hinton

Eyal Kazin

Tamara M. Davis

Chris Blake

Sarah Brough

Matthew Colless

Warrick J. Couch

Michael J. Drinkwater

Karl Glazebrook

Russell J. Jurek

David Parkinson

Kevin A. Pimbblet

Gregory B. Poole

Michael Pracy

David Woods

Crossref

Monthly Notices 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 Ωc h2, H(z), and DA(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

Brough, S 

UNSWorks

Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: Cosmological constraints

Legislative History: An Act to Amend the Date to Determine Age for Kindergarten Eligibility (HP284)(LD 367)

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