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

2012

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

Colless, Matthew, Beutler, Florian, Blake, Chris

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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/Mpc, 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.

Built on

Landy, S.D., & Szalay, A.S. 1993, ApJ
1993
Earlier work this paper cites.
Feldman, H.A., Kaiser, N., & Peacock, J.A. 1994, ApJ
1994
Earlier work this paper cites.
Jarrett, T.H., et al
2000
Earlier work this paper cites.
Blake, C. & Glazebrook, K. 2003, ApJ
2003
Earlier work this paper cites.
Seo, H.J., & Eisenstein, D.J. 2003, ApJ
2003
Earlier work this paper cites.

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Then

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