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

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper

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 Â± 3.2 km sâˆ’1 Mpcâˆ’1, achieving a 1Ïƒ precision of 5%. With improved analysis techniques, the planned wallaby (Hi) and taipan (optical) redshift surveys are predicted to measure H0 to 13% precision.

Original language	English
Title of host publication	Advancing the Physics of Cosmic Distances
Editors	Richard de Grijs
Place of Publication	Cambridge
Publisher	Cambridge University Press
Pages	319-322pp
DOIs	https://doi.org/10.1017/S1743921312021618
Publication status	Published - 2013
Event	Advancing the Physics of Cosmic Distances - Beijing, China, China Duration: 1 Jan 2013 → … http://journals.cambridge.org/action/displayIssue?jid=IAU&volumeId=8&seriesId=0&issueId=S289

Conference

Conference	Advancing the Physics of Cosmic Distances
Country/Territory	China
Period	1/01/13 → …
Other	27-31 Aug 2012
Internet address	http://journals.cambridge.org/action/displayIssue?jid=IAU&volumeId=8&seriesId=0&issueId=S289

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10.1017/S1743921312021618

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@inproceedings{1528083b09b74b81bb00f142e35f4477,

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 {\^A}± 3.2 km s{\^a}ˆ{\textquoteright}1 Mpc{\^a}ˆ{\textquoteright}1, achieving a 1{\"I}ƒ precision of 5\%. With improved analysis techniques, the planned wallaby (Hi) and taipan (optical) redshift surveys are predicted to measure H0 to 13\% precision.",

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

year = "2013",

doi = "10.1017/S1743921312021618",

language = "English",

pages = "319--322pp",

editor = "\{Richard de Grijs\}",

booktitle = "Advancing the Physics of Cosmic Distances",

publisher = "Cambridge University Press",

address = "United Kingdom",

note = "Advancing the Physics of Cosmic Distances ; Conference date: 01-01-2013",

url = "http://journals.cambridge.org/action/displayIssue?jid=IAU\&volumeId=8\&seriesId=0\&issueId=S289",

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T1 - Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys

AU - Colless, Matthew

AU - Beutler, Florian

AU - Blake, Chris

PY - 2013

Y1 - 2013

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 Â± 3.2 km sâˆ’1 Mpcâˆ’1, achieving a 1Ïƒ precision of 5%. With improved analysis techniques, the planned wallaby (Hi) and taipan (optical) redshift surveys are predicted to measure H0 to 13% 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 Â± 3.2 km sâˆ’1 Mpcâˆ’1, achieving a 1Ïƒ precision of 5%. With improved analysis techniques, the planned wallaby (Hi) and taipan (optical) redshift surveys are predicted to measure H0 to 13% precision.

U2 - 10.1017/S1743921312021618

DO - 10.1017/S1743921312021618

M3 - Conference Paper

SP - 319

EP - 322

BT - Advancing the Physics of Cosmic Distances

A2 - null, Richard de Grijs

PB - Cambridge University Press

CY - Cambridge

T2 - Advancing the Physics of Cosmic Distances

Y2 - 1 January 2013

ER -

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

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