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

Matthew Colless, Florian Beutler, Chris Blake

Research output: Contribution to journalArticlepeer-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 languageEnglish
Pages (from-to)319-322
Number of pages4
JournalProceedings of the International Astronomical Union
Volume8
Issue numberS289
DOIs
Publication statusPublished - 26 Feb 2013

Keywords

  • astro-ph.CO

Fingerprint

Dive into the research topics of 'Measuring H<sub>0</sub> from the 6dF Galaxy Survey and future low-redshift surveys'. Together they form a unique fingerprint.

Cite this