Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys

Matthew Colless; Florian Beutler; Chris Blake

doi:10.1017/S1743921312021618

Measuring H₀ from the 6dF Galaxy Survey and future low-redshift surveys

Matthew Colless, Florian Beutler, Chris Blake

Institute of Cosmology & Gravitation

Research output: Contribution to journal › Article › peer-review

Abstract

Baryon acoustic oscillations (BAO) at low redshift provide a precise and largely model-independent way to measure the Hubble constant, H₀. The 6dF Galaxy Survey measurement of the BAO scale gives a value of H₀ = 67 ± 3.2 km s ^-1 Mpc^-1, achieving a 1-sigma precision of 5%. With improved analysis techniques, the planned WALLABY (Hi) and TAIPAN (optical) redshift surveys are predicted to measure H₀ to 1-3% precision.

Original language	English
Pages (from-to)	319-322
Number of pages	4
Journal	Proceedings of the International Astronomical Union
Volume	8
Issue number	S289
DOIs	https://doi.org/10.1017/S1743921312021618
Publication status	Published - 26 Feb 2013

Keywords

astro-ph.CO

Access to Document

10.1017/S1743921312021618

Cite this

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title = "Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys",

abstract = "Baryon acoustic oscillations (BAO) at low redshift provide a precise and largely model-independent way to measure the Hubble constant, H0. The 6dF Galaxy Survey measurement of the BAO scale gives a value of H0 = 67 ± 3.2 km s -1 Mpc-1, achieving a 1-sigma precision of 5%. With improved analysis techniques, the planned WALLABY (Hi) and TAIPAN (optical) redshift surveys are predicted to measure H0 to 1-3% precision.",

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author = "Matthew Colless and Florian Beutler and Chris Blake",

note = "Proceedings of IAU Symposium 289, {"}Advancing the Physics of Cosmic Distances{"}, Richard de Grijs & Giuseppe Bono (eds), 2012, 4pp",

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AU - Colless, Matthew

AU - Beutler, Florian

AU - Blake, Chris

N1 - Proceedings of IAU Symposium 289, "Advancing the Physics of Cosmic Distances", Richard de Grijs & Giuseppe Bono (eds), 2012, 4pp

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N2 - Baryon acoustic oscillations (BAO) at low redshift provide a precise and largely model-independent way to measure the Hubble constant, H0. The 6dF Galaxy Survey measurement of the BAO scale gives a value of H0 = 67 ± 3.2 km s -1 Mpc-1, achieving a 1-sigma precision of 5%. With improved analysis techniques, the planned WALLABY (Hi) and TAIPAN (optical) redshift surveys are predicted to measure H0 to 1-3% precision.

AB - Baryon acoustic oscillations (BAO) at low redshift provide a precise and largely model-independent way to measure the Hubble constant, H0. The 6dF Galaxy Survey measurement of the BAO scale gives a value of H0 = 67 ± 3.2 km s -1 Mpc-1, achieving a 1-sigma precision of 5%. With improved analysis techniques, the planned WALLABY (Hi) and TAIPAN (optical) redshift surveys are predicted to measure H0 to 1-3% precision.

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